{"id":34192,"date":"1998-01-01T00:00:00","date_gmt":"1998-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/galaxias-con-formacion-estelar-intensa-sistemas-binarios-y-emision-x\/"},"modified":"1998-01-01T00:00:00","modified_gmt":"1998-01-01T00:00:00","slug":"galaxias-con-formacion-estelar-intensa-sistemas-binarios-y-emision-x","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/galaxias-con-formacion-estelar-intensa-sistemas-binarios-y-emision-x\/","title":{"rendered":"Galaxias con formacion estelar intensa: sistemas binarios y emision x."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Miguel Cervi\u00f1o Saavedra <\/strong><\/h2>\n<p>En este trabajo se desarrollan modelos de s\u00edntesis evolutiva de poblaci\u00f3n estelar en los que se incluye la evoluci\u00f3n de sistemas binarios en un rango de edades de 0 a 30 millones de a\u00f1os desde la formaci\u00f3n de las estrellas masivas del brote.  el trabajo extiende los modelos presentados por mas-hesse &amp; kunth (1991, a&amp;ass, 88, 317) y cervi\u00f1o &amp; mas-hesse (1994 a&amp;a, 284, 749) incorporando la emisi\u00f3n en rayos x y la influencia de sistemas binarios en la evoluci\u00f3n del brote de formaci\u00f3n estelar, obteniendose la emisi\u00f3n multirrango desde radio a rayos x de galaxias que han sufrido este tipo de procesos. Tambi\u00e9n se han actualizado los valores utilizados en versiones anteriores del c\u00f3digo para los casos que haya sido necesario. Dado que tanto la emisi\u00f3n en rayos x como la influencia de sistemas binarios no ha sido estudiada anteriormente se ha hecho un especial \u00e9nfasis en estos aspectos.  por \u00faltimo hemos aplicado los modelos a un conjunto de galaxias con distintos grados de actividad (galaxias con formaci\u00f3n estelar y n\u00facleos activos de galaxias) para discriminar cual es el origen de la emisi\u00f3n en los distintos rangos de energ\u00eda del continuo multirrango.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Galaxias con formacion estelar intensa: sistemas binarios y emision x.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Galaxias con formacion estelar intensa: sistemas binarios y emision x. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Miguel Cervi\u00f1o Saavedra <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Complutense de Madrid<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1998<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n<h3>Direcci\u00f3n y tribunal<\/h3>\n<ul>\n<li><strong>Director de la tesis<\/strong>\n<ul>\n<li>Jos\u00e9 Miguel Mas Hesse<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Jose Campos Gutierrez <\/li>\n<li>\u00e1lvaro Gim\u00e9nez Ca\u00f1ete (vocal)<\/li>\n<li>Jaime Zamorano Calvo (vocal)<\/li>\n<li>Daniel Kunth (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Miguel Cervi\u00f1o Saavedra En este trabajo se desarrollan modelos de s\u00edntesis evolutiva de poblaci\u00f3n estelar en los [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"","site-content-style":"default","site-sidebar-style":"default","ast-global-header-display":"","ast-banner-title-visibility":"","ast-main-header-display":"","ast-hfb-above-header-display":"","ast-hfb-below-header-display":"","ast-hfb-mobile-header-display":"","site-post-title":"","ast-breadcrumbs-content":"","ast-featured-img":"","footer-sml-layout":"","theme-transparent-header-meta":"","adv-header-id-meta":"","stick-header-meta":"","header-above-stick-meta":"","header-main-stick-meta":"","header-below-stick-meta":"","astra-migrate-meta-layouts":"default","ast-page-background-enabled":"default","ast-page-background-meta":{"desktop":{"background-color":"var(--ast-global-color-4)","background-image":"","background-repeat":"repeat","background-position":"center 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