{"id":55379,"date":"2006-07-11T00:00:00","date_gmt":"2006-07-11T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/composicion-quimica-de-estrellas-que-orbitan-alrededor-de-agujeros-negros-y-estrellas-de-neutrones\/"},"modified":"2006-07-11T00:00:00","modified_gmt":"2006-07-11T00:00:00","slug":"composicion-quimica-de-estrellas-que-orbitan-alrededor-de-agujeros-negros-y-estrellas-de-neutrones","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/espectroscopia-astrofisica\/composicion-quimica-de-estrellas-que-orbitan-alrededor-de-agujeros-negros-y-estrellas-de-neutrones\/","title":{"rendered":"Composicion quimica de estrellas que orbitan alrededor de agujeros negros y estrellas de neutrones"},"content":{"rendered":"<h2>Tesis doctoral de <strong>  Gonzalez Hernandez Jonay Isai <\/strong><\/h2>\n<p>En esta tesis se ha llevado a cabo el estudio de abundancias qu\u00edmicas de las estrellas secundarias en sistemas binarios de rayos x de masa peque\u00f1a con el fin de extraer informaci\u00f3n sobre la nucleos\u00edntesis en estrellas masivas y los procesos de formaci\u00f3n de objetos compactos, tanto agujeros negros como estrellas de neutrones . Las estrellas secundarias pudieron haber capturado parte del material eyectado en las explosiones de supernova que probablemente dieron lugar a la formaci\u00f3n de los objetos compactos.  Para llevar a cabo este proyecto se realizaron observaciones espectrosc\u00f3picas en telescopios de clase 8-10 metros, vlt y keck, con espectr\u00f3grafos de resoluci\u00f3n intermedia-alta. Los resultados obtenidos permiten establecer restricciones a los par\u00e1metros involucrados en las explosiones de supernova y definir de forma preliminar una relaci\u00f3n entre la masa de los objetos compactos y sus progenitores.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Composicion quimica de estrellas que orbitan alrededor de agujeros negros y estrellas de neutrones<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Composicion quimica de estrellas que orbitan alrededor de agujeros negros y estrellas de neutrones <\/li>\n<li><strong>Autor:<\/strong>\u00a0  Gonzalez Hernandez Jonay Isai <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 07\/11\/2006<\/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>Rafael Rebolo Lopez<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: artemio Herrero davo <\/li>\n<li> Ruiz lapuente m. pilar (vocal)<\/li>\n<li> Mirabel miquele i. felix (vocal)<\/li>\n<li>Carlos Antonio Abia ladron de guevara (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Gonzalez Hernandez Jonay Isai En esta tesis se ha llevado a cabo el estudio de abundancias qu\u00edmicas [&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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