{"id":793,"date":"2017-06-10T08:21:56","date_gmt":"2017-06-10T08:21:56","guid":{"rendered":"http:\/\/xtratheme.comlawyers\/?page_id=4"},"modified":"2025-11-22T21:08:52","modified_gmt":"2025-11-22T21:08:52","slug":"home","status":"publish","type":"page","link":"https:\/\/rgb.iaa.es\/es\/","title":{"rendered":"Inicio"},"content":{"rendered":"<div class=\"wpb-content-wrapper\"><p>[vc_row][vc_column][rev_slider_vc alias=\u00bbspanish\u00bb][\/vc_column][\/vc_row][vc_row][vc_column offset=\u00bbvc_col-lg-6&#8243;]<div class=\"cz_wrap clr\"><div id=\"cz_19238\" class=\"cz_19238 cz_title clr cz_title_pos_inline\"><style class=\"cz_d_css\" data-noptimize>#cz_19238 .cz_title_content{padding-left:10px}<\/style><style class=\"cz_t_css\" data-noptimize>@media screen and (max-width:768px){#cz_19238 .cz_title_content{margin-top:90px}}<\/style><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 38px;\">Bienvenido a la web de<br \/>\n<\/span><\/h3>\n<h1><span style=\"font-size: 38px;\"><span style=\"color: #d8ae76;\">Rub\u00e9n Garc\u00eda-Benito<\/span><\/span><\/h1>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 50px\"><\/div>[vc_column_text]\u00bfQuieres saber c\u00f3mo se forman y evolucionan las galaxias?<\/p>\n<p>Disfruta de este magn\u00edfico documental acerca de nuestro trabajo en el cartografiado CALIFA.[\/vc_column_text][\/vc_column][vc_column offset=\u00bbvc_col-lg-6&#8243;]<div class=\"clr cz_parallax_v_20\"><div id=\"cz_19870\" class=\"cz_19870 cz_video_popup clr cz_video_popup_bl\"><style class=\"cz_d_css\" data-noptimize>#cz_19870 span{color:#0a0505;background-color:#d8ae76;padding:18px;border-radius:4px}#cz_19870 .cz_vp_inner{color:#d8ae76;border-radius:4px}<\/style><div><div class=\"cz_vp_c\"><a href=\"https:\/\/www.youtube.com\/watch?v=H9SLRnUxkOA\"><img decoding=\"async\" width=\"1000\" height=\"884\" src=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/RGB-IAA-video-cover-small.png\" class=\"attachment-full\" alt=\"RGB IAA video cover small\" title=\"RGB-IAA-video-cover-small\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/RGB-IAA-video-cover-small.png 1000w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/RGB-IAA-video-cover-small-300x265.png 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/RGB-IAA-video-cover-small-768x679.png 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/RGB-IAA-video-cover-small-600x530.png 600w\" sizes=\"auto, (max-width: 1000px) 100vw, 1000px\" loading=\"lazy\" \/><div class=\"cz_vp_inner\"><span><i class=\"fa fa-play\"><\/i><\/span><h4>Paleontolog\u00eda Gal\u00e1ctica<small>Ver v\u00eddeo<\/small><\/h4><\/div><\/a><\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.tilt !== \"undefined\" ) {Codevz_Plus.tilt();}Codevz_Plus.inline_video( true );Codevz_Plus.parallax();jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div>[\/vc_column][\/vc_row][vc_row full_width=\u00bbstretch_row\u00bb parallax=\u00bbcontent-moving-fade\u00bb parallax_image=\u00bb1062&#8243;][vc_column]<div class=\"cz_gap clr  hide_on_tablet hide_on_mobile\" style=\"height: 40px\"><\/div><div class=\"cz_gap show_on_tablet clr  show_only_tablet\" style=\"height: 30px\"><\/div><div class=\"cz_gap show_on_mobile clr\" style=\"height: 30px\"><\/div><div class=\"cz_wrap clr\"><div id=\"cz_48389\" class=\"cz_48389 cz_title clr cz_title_pos_inline\"><style class=\"cz_d_css\" data-noptimize>#cz_48389 .cz_title_content{padding-left:10px}<\/style><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 38px;\">L\u00edneas de <\/span><span style=\"font-size: 38px;\"><span style=\"color: #d8ae76;\">Investigaci\u00f3n<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 20px\"><\/div><div class=\"cz_wrap clr\"><div id=\"cz_59045\" class=\"cz_59045 cz_tabs clr cz_tabs_vl cz_tabs_is_v cz_tabs_flash\"><style class=\"cz_d_css\" data-noptimize>#cz_59045 .cz_tabs_nav div{border-style:solid;border-width:1px;border-color:rgba(255,255,255,0.1);border-radius:4px}#cz_59045 .cz_tab_a{border-bottom-style:solid;border-color:rgba(255,255,255,0.1);border-top-style:solid;border-right-style:solid;border-left-style:solid;padding:10px 20px 10px 20px;border-width:0px 0px 1px 0px;margin-bottom:0px}#cz_59045 .cz_tab_a.active, #cz_59045 .cz_tab_a.cz_active{background-color:#d8ae76;padding-left:26px;color:#191919}<\/style><style class=\"cz_m_css\" data-noptimize>@media screen and (max-width:480px){#cz_59045 .cz_tab{padding-right:0px;padding-left:0px}}<\/style><div class=\"cz_tabs_content\"><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_67214\" href=\"#\"><i class=\"cz_tab_icon fa fa-angle-double-right mr8\"><\/i><span class=\"cz_tab_in_title\">M\u00e1s...<\/span><\/a><div id=\"cz_67214\" class=\"cz_tab\"><div>[vc_row_inner][vc_column_inner width=\u00bb1\/2&#8243;]<div class=\"cz_wrap clr\"><div class=\"clr\"><ul id=\"cz_78973\" class=\"cz_78973 cz_stylish_list clr cz_sl_icon_hover_zoom_in\"><style class=\"cz_d_css\" data-noptimize>#cz_78973 li{font-weight:500;font-size:18px}#cz_78973 i{color:#111111;background-color:#d8ae76;margin-right:16px;border-style:dashed;border-width:1px;border-color:#d8ae76;border-radius:4px}<\/style><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2009A%26A...497...53P\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Polar Ring Galaxies<\/span><\/div><\/a><\/li><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Blue Compact Dwarf Galaxies<\/span><\/div><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Star Formation Histories<\/span><\/div><\/a><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Sinolog\u00eda<\/span><\/div><\/a><\/li><\/ul><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div>[\/vc_column_inner][vc_column_inner width=\u00bb1\/2&#8243;]<div class=\"cz_wrap clr\"><div class=\"clr\"><ul id=\"cz_46595\" class=\"cz_46595 cz_stylish_list clr cz_sl_icon_hover_zoom_in\"><style class=\"cz_d_css\" data-noptimize>#cz_46595 li{font-weight:500;font-size:18px}#cz_46595 i{color:#d8ae76;margin-right:16px;border-style:dashed;border-width:1px;border-color:#d8ae76;border-radius:4px}<\/style><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Long-slit spectroscopy<\/span><\/div><\/li><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Integral Field Spectroscopy<\/span><\/div><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Color Magnitude Diagrams<\/span><\/div><\/a><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Musicolog\u00eda cultural<\/span><\/div><\/a><\/li><\/ul><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div>[\/vc_column_inner][\/vc_row_inner]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_67214\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_82361\" href=\"#\"><i class=\"cz_tab_icon fas fa-music mr8\"><\/i><span class=\"cz_tab_in_title\">Sonificaci\u00f3n<\/span><\/a><div id=\"cz_82361\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_73679\" class=\"cz_73679 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Soni<span style=\"color: #d8ae76;\">ficaci\u00f3n<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 40px\"><\/div>[vc_column_text css=\u00bb\u00bb]<img loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-2654 alignleft\" src=\"http:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-300x235.jpg\" alt=\"\" width=\"300\" height=\"235\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-300x235.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-1024x803.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-768x602.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-1536x1204.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-2048x1606.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-600x470.jpg 600w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/>La sonificaci\u00f3n ofrece una v\u00eda alternativa para explorar los datos mediante la traducci\u00f3n de informaci\u00f3n cuantitativa en sonido. Esta t\u00e9cnica proporciona un medio intuitivo para identificar estructuras, tendencias y anomal\u00edas que pueden resultar dif\u00edciles de discernir visualmente o cuya interpretaci\u00f3n puede beneficiarse de enfoques multimodales.<\/p>\n<p>Por ejemplo, he aplicado esta t\u00e9cnica a conjuntos de datos de espectroscop\u00eda de campo integral para facilitar la exploraci\u00f3n de cubos de datos complejos. La sonificaci\u00f3n tambi\u00e9n es un medio muy efectivo para comunicar resultados astron\u00f3micos a p\u00fablicos m\u00e1s amplios, haciendo que los procesos f\u00edsicos subyacentes sean m\u00e1s accesibles e inclusivos.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_82361\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_105281\" href=\"#\"><i class=\"cz_tab_icon fa fa-star mr8\"><\/i><span class=\"cz_tab_in_title\">Regiones HII<\/span><\/a><div id=\"cz_105281\" class=\"cz_tab\"><div>[vc_hoverbox image=\u00bb1016&#8243; primary_title=\u00bbRegiones HII\u00bb hover_title=\u00bb\u00bb shape=\u00bbround\u00bb hover_background_color=\u00bbcustom\u00bb el_width=\u00bb80&#8243; css_animation=\u00bbappear\u00bb hover_custom_background=\u00bbrgba(216,174,118,0.95)\u00bb]<\/p>\n<p style=\"text-align: center;\">Las <strong>regiones HII<\/strong> son importantes trazadores de formaci\u00f3n estelar en la evoluci\u00f3n qu\u00edmica de las galaxias y pueden ser utilizadas como velas est\u00e1ndar para estimar distancias cosmol\u00f3gicas. De igual forma, son uno de los mejores indicadores de las condiciones que conducen a la <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2011AJ....141..126G\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">formaci\u00f3n masiva de estrellas<\/a>.<\/p>\n<p>[\/vc_hoverbox]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_105281\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_62950\" href=\"#\"><i class=\"cz_tab_icon fa czico-041-physics mr8\"><\/i><span class=\"cz_tab_in_title\">Nebulosas<\/span><\/a><div id=\"cz_62950\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_100977\" class=\"cz_100977 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Gas y <span style=\"color: #d8ae76;\">Nebulosas<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 40px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1018 alignleft\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-300x285.jpg\" alt=\"\" width=\"357\" height=\"339\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-300x285.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-1024x973.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-768x729.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-1536x1459.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-2048x1945.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-600x570.jpg 600w\" sizes=\"auto, (max-width: 357px) 100vw, 357px\" \/><\/p>\n<p>Las l\u00edneas de emisi\u00f3n permiten estudiar las nebulosas gaseosas, sus propiedades f\u00edsicas y su composici\u00f3n qu\u00edmica.<\/p>\n<p>Las estrellas calientes en las <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2010MNRAS.408.2234G\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">regiones de formaci\u00f3n de estrellas j\u00f3venes<\/a> crean espectros hermosos llenos de intensas l\u00edneas.<\/p>\n<p>Por otro lado, algunas estrellas moribundas crean asombrosas c\u00e1scaras expansivas de gas luminoso. En trabajos recientes he estado usando <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2015ApJ...815...69F\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">nebulosas planetarias<\/a> como trazadores para estudiar la qu\u00edmica, cinem\u00e1tica y contenido estelar de las subestructuras M31. Tambi\u00e9n son uno de los mejores candidatos que pueden proporcionar tanto velocidades como mediciones muy precisas de abundancia de elementos como O, He, Ne, N, Ar, y S.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_62950\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_70266\" href=\"#\"><i class=\"cz_tab_icon fa fa-star-o mr8\"><\/i><span class=\"cz_tab_in_title\">Formaci\u00f3n Estelar<\/span><\/a><div id=\"cz_70266\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_94754\" class=\"cz_94754 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Formaci\u00f3n <span style=\"color: #d8ae76;\">Estelar<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 10px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1007 alignright\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-300x200.jpg\" alt=\"\" width=\"359\" height=\"239\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-300x200.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-1024x683.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-768x512.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-1536x1024.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-2048x1366.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-600x400.jpg 600w\" sizes=\"auto, (max-width: 359px) 100vw, 359px\" \/><\/p>\n<div class=\"page\" title=\"Page 21\">\n<div class=\"section\">\n<div class=\"layoutArea\">\n<div class=\"column\">\n<p>La formaci\u00f3n estelar es un proceso continuo en el universo local. La mayor\u00eda de la luz y los metales se producen en las m\u00e1s masivas de las estrellas reci\u00e9n formadas. Las regiones m\u00e1s extremas que forman estrellas masivas se denominan a menudo <em>starburst<\/em>. En el universo local representan aproximadamente una cuarta parte de toda la formaci\u00f3n estelar y esta fracci\u00f3n puede ser mayor en el universo m\u00e1s joven.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_70266\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_73160\" href=\"#\"><i class=\"cz_tab_icon fa fa-star mr8\"><\/i><span class=\"cz_tab_in_title\">Formaci\u00f3n y Evoluci\u00f3n de Galaxias<\/span><\/a><div id=\"cz_73160\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><h2 id=\"cz_47092\" data-time=\"4000\" class=\"cz_47092 cz_headline rotate-1\"><style class=\"cz_d_css\" data-noptimize>#cz_47092 .cz_words-wrapper{color:#d8ae76}<\/style><span class=\"cz_before_text\">Galaxias:<\/span><span class=\"cz_words-wrapper\"><b class=\"is-visible\">Formaci\u00f3n<\/b><b class=\"is-hidden\">Evoluci\u00f3n<\/b><\/span><\/h2><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.animated_text !== \"undefined\" ) {Codevz_Plus.animated_text();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr  hide_on_tablet hide_on_mobile\" style=\"height: 30px\"><\/div><div class=\"cz_gap show_on_tablet clr  show_only_tablet\" style=\"height: 20px\"><\/div><div class=\"cz_gap show_on_mobile clr\" style=\"height: 20px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1017 alignleft\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-268x300.jpg\" alt=\"\" width=\"340\" height=\"380\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-268x300.jpg 268w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-915x1024.jpg 915w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-768x860.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-1372x1536.jpg 1372w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-1830x2048.jpg 1830w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-600x672.jpg 600w\" sizes=\"auto, (max-width: 340px) 100vw, 340px\" \/><\/p>\n<p>Las galaxias son una mezcla compleja de estrellas, gas interestelar, polvo y materia oscura, distribuidas en el bulgo, el disco y el halo. La estructura y din\u00e1mica actual de estos subcomponentes de las galaxias est\u00e1n \u00edntimamente ligadas a su ensamblaje y evoluci\u00f3n a lo largo de la edad del Universo.<\/p>\n<p>Durante los \u00faltimos a\u00f1os he estado trabajando en un <a href=\"https:\/\/www.iaa.csic.es\/~rosa\/3DUniverse\/3DUniverse\/3DUniverse\/3DUniverse.html\" target=\"_blank\" rel=\"noopener noreferrer\">proyecto<\/a> cuyo objetivo es encontrar evidencias observacionales para validar o rechazar los diferentes modelos de formaci\u00f3n y evoluci\u00f3n de galaxias, resolviendo en el tiempo y en el espacio las <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017A%26A...608A..27G\" target=\"_blank\" rel=\"noopener noreferrer\">propiedades de las poblaciones estelares<\/a> de galaxias en el Universo local, utilizando datos de \u00faltima generaci\u00f3n del <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015A%26A...576A.135G\" target=\"_blank\" rel=\"noopener noreferrer\">cartografiado CALIFA<\/a>.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_73160\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><\/div><\/div><div class=\"cz_tabs_org hide\"><div id=\"cz_59045\" class=\"cz_59045 cz_tabs clr cz_tabs_vl cz_tabs_is_v cz_tabs_flash\"><style class=\"cz_d_css\" data-noptimize>#cz_59045 .cz_tabs_nav div{border-style:solid;border-width:1px;border-color:rgba(255,255,255,0.1);border-radius:4px}#cz_59045 .cz_tab_a{border-bottom-style:solid;border-color:rgba(255,255,255,0.1);border-top-style:solid;border-right-style:solid;border-left-style:solid;padding:10px 20px 10px 20px;border-width:0px 0px 1px 0px;margin-bottom:0px}#cz_59045 .cz_tab_a.active, #cz_59045 .cz_tab_a.cz_active{background-color:#d8ae76;padding-left:26px;color:#191919}<\/style><style class=\"cz_m_css\" data-noptimize>@media screen and (max-width:480px){#cz_59045 .cz_tab{padding-right:0px;padding-left:0px}}<\/style><div class=\"cz_tabs_content\"><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_67214\" href=\"#\"><i class=\"cz_tab_icon fa fa-angle-double-right mr8\"><\/i><span class=\"cz_tab_in_title\">M\u00e1s...<\/span><\/a><div id=\"cz_67214\" class=\"cz_tab\"><div>[vc_row_inner][vc_column_inner width=\u00bb1\/2&#8243;]<div class=\"cz_wrap clr\"><div class=\"clr\"><ul id=\"cz_78973\" class=\"cz_78973 cz_stylish_list clr cz_sl_icon_hover_zoom_in\"><style class=\"cz_d_css\" data-noptimize>#cz_78973 li{font-weight:500;font-size:18px}#cz_78973 i{color:#111111;background-color:#d8ae76;margin-right:16px;border-style:dashed;border-width:1px;border-color:#d8ae76;border-radius:4px}<\/style><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2009A%26A...497...53P\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Polar Ring Galaxies<\/span><\/div><\/a><\/li><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Blue Compact Dwarf Galaxies<\/span><\/div><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Star Formation Histories<\/span><\/div><\/a><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa fa-check mr10\"><\/i><\/div><div><span>Sinolog\u00eda<\/span><\/div><\/a><\/li><\/ul><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div>[\/vc_column_inner][vc_column_inner width=\u00bb1\/2&#8243;]<div class=\"cz_wrap clr\"><div class=\"clr\"><ul id=\"cz_46595\" class=\"cz_46595 cz_stylish_list clr cz_sl_icon_hover_zoom_in\"><style class=\"cz_d_css\" data-noptimize>#cz_46595 li{font-weight:500;font-size:18px}#cz_46595 i{color:#d8ae76;margin-right:16px;border-style:dashed;border-width:1px;border-color:#d8ae76;border-radius:4px}<\/style><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Long-slit spectroscopy<\/span><\/div><\/li><li class=\"clr\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Integral Field Spectroscopy<\/span><\/div><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Color Magnitude Diagrams<\/span><\/div><\/a><\/li><li class=\"clr\"><a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2012MNRAS.423..406G\/abstract\" target=\"_blank\"><div class=\"cz_sl_icon\"><i class=\"fa czico-072-check-mark mr10\"><\/i><\/div><div><span>Musicolog\u00eda cultural<\/span><\/div><\/a><\/li><\/ul><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div>[\/vc_column_inner][\/vc_row_inner]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_67214\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_82361\" href=\"#\"><i class=\"cz_tab_icon fas fa-music mr8\"><\/i><span class=\"cz_tab_in_title\">Sonificaci\u00f3n<\/span><\/a><div id=\"cz_82361\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_73679\" class=\"cz_73679 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Soni<span style=\"color: #d8ae76;\">ficaci\u00f3n<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 40px\"><\/div>[vc_column_text css=\u00bb\u00bb]<img loading=\"lazy\" decoding=\"async\" class=\"size-medium wp-image-2654 alignleft\" src=\"http:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-300x235.jpg\" alt=\"\" width=\"300\" height=\"235\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-300x235.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-1024x803.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-768x602.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-1536x1204.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-2048x1606.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/rgb\/ngc2916-datacube-stamp-600x470.jpg 600w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/>La sonificaci\u00f3n ofrece una v\u00eda alternativa para explorar los datos mediante la traducci\u00f3n de informaci\u00f3n cuantitativa en sonido. Esta t\u00e9cnica proporciona un medio intuitivo para identificar estructuras, tendencias y anomal\u00edas que pueden resultar dif\u00edciles de discernir visualmente o cuya interpretaci\u00f3n puede beneficiarse de enfoques multimodales.<\/p>\n<p>Por ejemplo, he aplicado esta t\u00e9cnica a conjuntos de datos de espectroscop\u00eda de campo integral para facilitar la exploraci\u00f3n de cubos de datos complejos. La sonificaci\u00f3n tambi\u00e9n es un medio muy efectivo para comunicar resultados astron\u00f3micos a p\u00fablicos m\u00e1s amplios, haciendo que los procesos f\u00edsicos subyacentes sean m\u00e1s accesibles e inclusivos.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_82361\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_105281\" href=\"#\"><i class=\"cz_tab_icon fa fa-star mr8\"><\/i><span class=\"cz_tab_in_title\">Regiones HII<\/span><\/a><div id=\"cz_105281\" class=\"cz_tab\"><div>[vc_hoverbox image=\u00bb1016&#8243; primary_title=\u00bbRegiones HII\u00bb hover_title=\u00bb\u00bb shape=\u00bbround\u00bb hover_background_color=\u00bbcustom\u00bb el_width=\u00bb80&#8243; css_animation=\u00bbappear\u00bb hover_custom_background=\u00bbrgba(216,174,118,0.95)\u00bb]<\/p>\n<p style=\"text-align: center;\">Las <strong>regiones HII<\/strong> son importantes trazadores de formaci\u00f3n estelar en la evoluci\u00f3n qu\u00edmica de las galaxias y pueden ser utilizadas como velas est\u00e1ndar para estimar distancias cosmol\u00f3gicas. De igual forma, son uno de los mejores indicadores de las condiciones que conducen a la <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2011AJ....141..126G\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">formaci\u00f3n masiva de estrellas<\/a>.<\/p>\n<p>[\/vc_hoverbox]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_105281\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_62950\" href=\"#\"><i class=\"cz_tab_icon fa czico-041-physics mr8\"><\/i><span class=\"cz_tab_in_title\">Nebulosas<\/span><\/a><div id=\"cz_62950\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_100977\" class=\"cz_100977 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Gas y <span style=\"color: #d8ae76;\">Nebulosas<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 40px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1018 alignleft\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-300x285.jpg\" alt=\"\" width=\"357\" height=\"339\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-300x285.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-1024x973.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-768x729.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-1536x1459.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-2048x1945.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/nasa-89125-unsplash-600x570.jpg 600w\" sizes=\"auto, (max-width: 357px) 100vw, 357px\" \/><\/p>\n<p>Las l\u00edneas de emisi\u00f3n permiten estudiar las nebulosas gaseosas, sus propiedades f\u00edsicas y su composici\u00f3n qu\u00edmica.<\/p>\n<p>Las estrellas calientes en las <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2010MNRAS.408.2234G\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">regiones de formaci\u00f3n de estrellas j\u00f3venes<\/a> crean espectros hermosos llenos de intensas l\u00edneas.<\/p>\n<p>Por otro lado, algunas estrellas moribundas crean asombrosas c\u00e1scaras expansivas de gas luminoso. En trabajos recientes he estado usando <a href=\"https:\/\/ui.adsabs.harvard.edu\/abs\/2015ApJ...815...69F\/abstract\" target=\"_blank\" rel=\"noopener noreferrer\">nebulosas planetarias<\/a> como trazadores para estudiar la qu\u00edmica, cinem\u00e1tica y contenido estelar de las subestructuras M31. Tambi\u00e9n son uno de los mejores candidatos que pueden proporcionar tanto velocidades como mediciones muy precisas de abundancia de elementos como O, He, Ne, N, Ar, y S.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_62950\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_70266\" href=\"#\"><i class=\"cz_tab_icon fa fa-star-o mr8\"><\/i><span class=\"cz_tab_in_title\">Formaci\u00f3n Estelar<\/span><\/a><div id=\"cz_70266\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><div id=\"cz_94754\" class=\"cz_94754 cz_title clr cz_title_pos_inline\"><div class=\"cz_title_content\"><div class=\"cz_wpe_content\"><h3><span style=\"font-size: 32px;\">Formaci\u00f3n <span style=\"color: #d8ae76;\">Estelar<\/span><\/span><\/h3>\n<\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.title !== \"undefined\" ) {Codevz_Plus.title();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr \" style=\"height: 10px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1007 alignright\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-300x200.jpg\" alt=\"\" width=\"359\" height=\"239\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-300x200.jpg 300w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-1024x683.jpg 1024w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-768x512.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-1536x1024.jpg 1536w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-2048x1366.jpg 2048w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/billy-huynh-278252-unsplash-600x400.jpg 600w\" sizes=\"auto, (max-width: 359px) 100vw, 359px\" \/><\/p>\n<div class=\"page\" title=\"Page 21\">\n<div class=\"section\">\n<div class=\"layoutArea\">\n<div class=\"column\">\n<p>La formaci\u00f3n estelar es un proceso continuo en el universo local. La mayor\u00eda de la luz y los metales se producen en las m\u00e1s masivas de las estrellas reci\u00e9n formadas. Las regiones m\u00e1s extremas que forman estrellas masivas se denominan a menudo <em>starburst<\/em>. En el universo local representan aproximadamente una cuarta parte de toda la formaci\u00f3n estelar y esta fracci\u00f3n puede ser mayor en el universo m\u00e1s joven.<\/p>\n<\/div>\n<\/div>\n<\/div>\n<\/div>\n<p>[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_70266\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_wrap clr\"><a class=\"cz_tab_a hide\" data-tab=\"cz_73160\" href=\"#\"><i class=\"cz_tab_icon fa fa-star mr8\"><\/i><span class=\"cz_tab_in_title\">Formaci\u00f3n y Evoluci\u00f3n de Galaxias<\/span><\/a><div id=\"cz_73160\" class=\"cz_tab\"><div><div class=\"cz_wrap clr\"><h2 id=\"cz_47092\" data-time=\"4000\" class=\"cz_47092 cz_headline rotate-1\"><style class=\"cz_d_css\" data-noptimize>#cz_47092 .cz_words-wrapper{color:#d8ae76}<\/style><span class=\"cz_before_text\">Galaxias:<\/span><span class=\"cz_words-wrapper\"><b class=\"is-visible\">Formaci\u00f3n<\/b><b class=\"is-hidden\">Evoluci\u00f3n<\/b><\/span><\/h2><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {if( typeof Codevz_Plus.animated_text !== \"undefined\" ) {Codevz_Plus.animated_text();}jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr  hide_on_tablet hide_on_mobile\" style=\"height: 30px\"><\/div><div class=\"cz_gap show_on_tablet clr  show_only_tablet\" style=\"height: 20px\"><\/div><div class=\"cz_gap show_on_mobile clr\" style=\"height: 20px\"><\/div>[vc_column_text]<img loading=\"lazy\" decoding=\"async\" class=\" wp-image-1017 alignleft\" src=\"https:\/\/www.iaa.csic.es\/~rgb\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-268x300.jpg\" alt=\"\" width=\"340\" height=\"380\" srcset=\"https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-268x300.jpg 268w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-915x1024.jpg 915w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-768x860.jpg 768w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-1372x1536.jpg 1372w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-1830x2048.jpg 1830w, https:\/\/rgb.iaa.es\/wp-content\/uploads\/Imagenes\/astronomy\/john-fowler-330787-unsplash-600x672.jpg 600w\" sizes=\"auto, (max-width: 340px) 100vw, 340px\" \/><\/p>\n<p>Las galaxias son una mezcla compleja de estrellas, gas interestelar, polvo y materia oscura, distribuidas en el bulgo, el disco y el halo. La estructura y din\u00e1mica actual de estos subcomponentes de las galaxias est\u00e1n \u00edntimamente ligadas a su ensamblaje y evoluci\u00f3n a lo largo de la edad del Universo.<\/p>\n<p>Durante los \u00faltimos a\u00f1os he estado trabajando en un <a href=\"https:\/\/www.iaa.csic.es\/~rosa\/3DUniverse\/3DUniverse\/3DUniverse\/3DUniverse.html\" target=\"_blank\" rel=\"noopener noreferrer\">proyecto<\/a> cuyo objetivo es encontrar evidencias observacionales para validar o rechazar los diferentes modelos de formaci\u00f3n y evoluci\u00f3n de galaxias, resolviendo en el tiempo y en el espacio las <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2017A%26A...608A..27G\" target=\"_blank\" rel=\"noopener noreferrer\">propiedades de las poblaciones estelares<\/a> de galaxias en el Universo local, utilizando datos de \u00faltima generaci\u00f3n del <a href=\"http:\/\/adsabs.harvard.edu\/abs\/2015A%26A...576A.135G\" target=\"_blank\" rel=\"noopener noreferrer\">cartografiado CALIFA<\/a>.[\/vc_column_text]<\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( \"cz_73160\", true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><\/div><\/div><\/div><script>if( typeof Codevz_Plus !== \"undefined\" ) {setTimeout( function() {Codevz_Plus.tabs( false, true );jQuery( window ).trigger( \"scroll.codevz\" );}, 10 );}<\/script><\/div><div class=\"cz_gap clr  hide_on_tablet hide_on_mobile\" style=\"height: 120px\"><\/div><div class=\"cz_gap show_on_tablet clr  show_only_tablet\" style=\"height: 100px\"><\/div><div class=\"cz_gap show_on_mobile clr\" style=\"height: 50px\"><\/div>[\/vc_column][\/vc_row]<\/p>\n<\/div>","protected":false},"excerpt":{"rendered":"<p>\u00bfQuieres saber c\u00f3mo se forman y evolucionan las galaxias? Disfruta de &#8230; <\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"footnotes":""},"class_list":["post-793","page","type-page","status-publish","hentry"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v27.4 - https:\/\/yoast.com\/product\/yoast-seo-wordpress\/ -->\n<title>Rub\u00e9n Garc\u00eda-Benito: Astrophysicist @ IAA-CSIC<\/title>\n<meta name=\"description\" content=\"Rub\u00e9n Garc\u00eda-Benito&#039;s website | Astrophysicist @ IAA-CSIC\" \/>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/rgb.iaa.es\/es\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:locale:alternate\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Rub\u00e9n 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