{"id":46487,"date":"2019-11-13T17:54:58","date_gmt":"2019-11-13T17:54:58","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/sin-categoria\/fotometria-de-estrellas-am-evolucionadas\/"},"modified":"2019-11-13T17:54:58","modified_gmt":"2019-11-13T17:54:58","slug":"fotometria-de-estrellas-am-evolucionadas","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/fotometria-de-estrellas-am-evolucionadas\/","title":{"rendered":"Fotometria de estrellas am evolucionadas"},"content":{"rendered":"<h2>Tesis doctoral de <strong> Rafael Garrido Haba <\/strong><\/h2>\n<p>Algunas estrellas evolucionadas de tipo a metalicas se han observado fotometricamente para chequear su posible estabilidad pulsacional. No han sido encontradas variaciones dentro de  =0.003 hasta 0.006. Estos resultados conducen a una comparacion entre las estrellas am evolucionadas constantes y las estrellas   del que muestran anomalias de abundancia e inestabilidad pulsacional. Ademas han sido descubiertas dos nuevas estrellas pulsantes.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Fotometria de estrellas am evolucionadas<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Fotometria de estrellas am evolucionadas <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Rafael Garrido Haba <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Granada<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1980<\/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>Angel Rolland Quintanilla<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: LLuis Mas Franch <\/li>\n<li>Ram\u00f3n Canal Masgoret (vocal)<\/li>\n<li>Francisco Sanchez Martinez (vocal)<\/li>\n<li>Jos\u00e9 Ros Pallares (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Rafael Garrido Haba Algunas estrellas evolucionadas de tipo a metalicas se han observado fotometricamente para chequear su [&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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