{"id":2472,"date":"1994-01-01T00:00:00","date_gmt":"1994-01-01T00:00:00","guid":{"rendered":"https:\/\/www.deberes.net\/tesis\/1994\/01\/01\/parametros-fisicos-de-nubes-individuales-en-el-medio-interestelar-local\/"},"modified":"1994-01-01T00:00:00","modified_gmt":"1994-01-01T00:00:00","slug":"parametros-fisicos-de-nubes-individuales-en-el-medio-interestelar-local","status":"publish","type":"post","link":"https:\/\/www.deberes.net\/tesis\/astronomia-y-astrofisica\/parametros-fisicos-de-nubes-individuales-en-el-medio-interestelar-local\/","title":{"rendered":"Parametros fisicos de nubes individuales en el medio interestelar local."},"content":{"rendered":"<h2>Tesis doctoral de <strong> Joaquin Trapero Liener <\/strong><\/h2>\n<p>Utilizando espectros de alta resolucion (lamda\/incremento lamda = 810 elevado a 4) de la linea ki de absorcion interestelar, se estudian las nubes frias (t = 100 k) del medio interestelar local (mil). Se estiman distancias, tama\u00f1os, densidades, temperaturas y masas de las nubes.  una de las nubes, situada en perseo, se estudia mas detalladamente con observaciones en radio 21 cm, deduciendo una masa = 1300 mo, t = 35 pc y una distancia menos de 100 pc al sol. Ademas se utilizan observaciones en la linea na i de estrellas en la region escorpion-centauro lo que permite identificar nubes tibias (t = 8000 k), deduciendo sus parametros fisicos.  se discute el sentido de la variacion de n(nai)\/n(caii), efecto routly-spitzer, con una interpretacion distinta de la habitual.<\/p>\n<p>&nbsp;<\/p>\n<h3>Datos acad\u00e9micos de la tesis doctoral \u00ab<strong>Parametros fisicos de nubes individuales en el medio interestelar local.<\/strong>\u00ab<\/h3>\n<ul>\n<li><strong>T\u00edtulo de la tesis:<\/strong>\u00a0 Parametros fisicos de nubes individuales en el medio interestelar local. <\/li>\n<li><strong>Autor:<\/strong>\u00a0 Joaquin Trapero Liener <\/li>\n<li><strong>Universidad:<\/strong>\u00a0 La laguna<\/li>\n<li><strong>Fecha de lectura de la tesis:<\/strong>\u00a0 01\/01\/1994<\/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> Beckman Abramson Juan  Esteban<\/li>\n<\/ul>\n<\/li>\n<li><strong>Tribunal<\/strong>\n<ul>\n<li>Presidente del tribunal: Arne Ardeberg <\/li>\n<li>Francisco Garz\u00f3n L\u00f3pez (vocal)<\/li>\n<li>Eduard Salvador Sol\u00e9 (vocal)<\/li>\n<li>Jos\u00e9 Manuel V\u00edlchez Medina (vocal)<\/li>\n<\/ul>\n<\/li>\n<\/ul>\n<p>&nbsp;<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Tesis doctoral de Joaquin Trapero Liener Utilizando espectros de alta resolucion (lamda\/incremento lamda = 810 elevado a 4) de la [&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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