{"id":6114,"date":"1995-01-01T00:00:00","date_gmt":"1995-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/1995\/01\/01\/estudio-de-una-muestra-completa-de-galaxias-con-emision-en-h-alfa\/"},"modified":"1995-01-01T00:00:00","modified_gmt":"1995-01-01T00:00:00","slug":"estudio-de-una-muestra-completa-de-galaxias-con-emision-en-h-alfa","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/estudio-de-una-muestra-completa-de-galaxias-con-emision-en-h-alfa\/","title":{"rendered":"Estudio de una muestra completa de galaxias con emision en h-alfa."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Jes\u00fas Gallego Maestro <\/strong><\/h2>\n<p>Este trabajo consiste en caracterizar la muestra de galaxias con emision en halfa obtenida de la exploracion ucm. En total 272 objetos hasta un desplazamiento al rojo de 0.045 analizados espectroscopicamente. Cada uno de ellos fue clasificado segun ocho tipos espectroscopicos.  principalmente (47%) se trata de galaxias con intensos procesos de formacion estelar. Por otro lado, se ha encontrado un 43% de objetos de baja ionizacion que no se detectan con otras tecnicas. Los diferentes tipos observados forman una suave gradacion de procesos de formacion estelar en la que la metalicidad y el parametro de ionizacion son los parametros fundamentales. En contra de los postulados por algunos autores no se ha encontrado ninguna galaxia de metalicidad menor a los valores conocidos. Las galaxias estudiadas se presentan con mayor frecuencia en zonas de densidad de galaxias intermedia.  la funcion de luminosidad obtenida proporciona restricciones observacionales importantes a las teorias de formacion y evolucion de galaxias.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Estudio de una muestra completa de galaxias con emision en h-alfa.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Estudio de una muestra completa de galaxias con emision en h-alfa. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Jes\u00fas Gallego Maestro <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 Complutense de Madrid<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1995<\/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>Jaime Zamorano Calvo<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Manuel Rego Fernandez <\/li>\n<li> Rodriguez Espinosa Jos\u00e9 Miguel (vocal)<\/li>\n<li>Kurt Birkle (vocal)<\/li>\n<li>Rosario Gonz\u00e1lez Riestra (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Jes\u00fas Gallego Maestro Este trabajo consiste en caracterizar la muestra de galaxias con emision en halfa obtenida [&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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