{"id":11058,"date":"2019-05-08T09:55:49","date_gmt":"2019-05-08T12:55:49","guid":{"rendered":"https:\/\/www.iar.unlp.edu.ar\/?p=11058"},"modified":"2026-03-12T13:07:35","modified_gmt":"2026-03-12T13:07:35","slug":"coloquio-lydia-cidale","status":"publish","type":"post","link":"https:\/\/www.iar.unlp.edu.ar\/index.php\/2019\/05\/08\/coloquio-lydia-cidale\/","title":{"rendered":"Nuevas soluciones de vientos impulsados por radiaci\u00f3n"},"content":{"rendered":"<div><b>Expositor:<\/b> Lydia Cidale<\/div>\n<div><\/div>\n<div><b>T\u00edtulo: <\/b>Nuevas soluciones de vientos impulsados por radiaci\u00f3n<\/div>\n<div><span lang=\"es\" tabindex=\"0\">\u00a0<\/span><\/div>\n<div><span lang=\"es\" tabindex=\"0\"><b>Resumen: <\/b>La teor\u00eda cl\u00e1sica de los vientos estelares impulsados por radiaci\u00f3n <\/span><span lang=\"es\" tabindex=\"0\">explica razonablemente bien las condiciones observadas\u00a0 en los vientos estelares (p\u00e9rdida de masa y<\/span><span lang=\"es\" tabindex=\"0\"> velocidad terminal) de las estrellas supergigantes masivas. Sin embargo,\u00a0<\/span><span lang=\"es\" tabindex=\"0\"> todav\u00eda se encuentran diferencias entre los par\u00e1metros de viento predichos por<\/span><span lang=\"es\" tabindex=\"0\"> la teor\u00eda y aquellos observados en las estrellas B tard\u00edas y de tipo A.<\/span><span lang=\"es\" tabindex=\"0\"> La inclusi\u00f3n de la rotaci\u00f3n en las ecuaciones trajo un notable<\/span><span lang=\"es\" tabindex=\"0\"> avance en el desarrollo de la teor\u00eda de los vientos estelares. Actualmente podemos identificar\u00a0 <\/span><span lang=\"es\" tabindex=\"0\">tres reg\u00edmenes de vientos estacionarios. D<\/span><span lang=\"es\" tabindex=\"0\">iscutimos estas <\/span><span lang=\"es\" tabindex=\"0\">soluciones hidrodin\u00e1micas en el contexto de las observaciones de las estrellas supergigantes. <\/span><\/div>\n<p>13:30<\/p>\n<p>Aula del IAR<\/p>\n","protected":false},"excerpt":{"rendered":"<p>Expositor: Lydia Cidale T\u00edtulo: Nuevas soluciones de vientos impulsados por radiaci\u00f3n \u00a0 Resumen: La teor\u00eda cl\u00e1sica de los vientos estelares impulsados por radiaci\u00f3n explica razonablemente bien las condiciones observadas\u00a0 en &#8230;<\/p>\n","protected":false},"author":3,"featured_media":25277,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[14],"tags":[],"class_list":["post-11058","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-coloquios"],"_links":{"self":[{"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/posts\/11058","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/users\/3"}],"replies":[{"embeddable":true,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/comments?post=11058"}],"version-history":[{"count":1,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/posts\/11058\/revisions"}],"predecessor-version":[{"id":22513,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/posts\/11058\/revisions\/22513"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/media\/25277"}],"wp:attachment":[{"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/media?parent=11058"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/categories?post=11058"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.iar.unlp.edu.ar\/index.php\/wp-json\/wp\/v2\/tags?post=11058"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}