{"id":30,"date":"2018-04-20T14:32:45","date_gmt":"2018-04-20T14:32:45","guid":{"rendered":"http:\/\/auditore.cab.inta-csic.es\/masivas\/?page_id=30"},"modified":"2025-08-07T15:43:56","modified_gmt":"2025-08-07T15:43:56","slug":"projects","status":"publish","type":"page","link":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/projects\/","title":{"rendered":"Principal research lines"},"content":{"rendered":"\n<p>Massive stars are fundamental agents of the Universe at galactic-scale. They are mighty sources that ionize and shape the interstellar medium. Their death as supernovae can outshine entire galaxies and releases a wealth of metals synthesized in the stellar interior enriching the Universe. Either as basic ingredients or probes, massive stars are crucial to understand a variety of phenomena in Astrophysics.<\/p>\n\n\n\n<p>Within the Massive Star group at the CAB we focus our interests around complementary research lines focused on:<\/p>\n\n\n\n<ul class=\"wp-block-list\">\n<li><a href=\"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/low-z-massive-stars\/\" data-type=\"page\" data-id=\"135\">The physics of very low metallicity (low-Z) massive stars<\/a>,<\/li>\n\n\n\n<li><a href=\"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/ir-spectroscopy-of-mw-massive-stars\/\" data-type=\"page\" data-id=\"150\">Multiwavelength spectroscopic studies of massive stars<\/a> and<\/li>\n\n\n\n<li><a href=\"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/advanced-stages-of-massive-stars-evolution\/\" data-type=\"page\" data-id=\"164\">The advanced stages of massive star evolution<\/a><\/li>\n<\/ul>\n\n\n\n<p><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Massive stars are fundamental agents of the Universe at galactic-scale. They are mighty sources that ionize and shape the interstellar medium. Their death as supernovae can outshine entire galaxies and releases a wealth of metals synthesized in the stellar interior enriching the Universe. Either as basic ingredients or probes, massive stars are crucial to understand a variety of phenomena in Astrophysics. Within the Massive Star group at the CAB we focus our interests around complementary research lines focused on:<\/p>\n<a class=\"more-link\" rel=\"nofollow\" href=\"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/projects\/\">[Read More...]<\/a>","protected":false},"author":76,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"ngg_post_thumbnail":0,"footnotes":""},"class_list":["post-30","page","type-page","status-publish","hentry"],"_links":{"self":[{"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/pages\/30","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/users\/76"}],"replies":[{"embeddable":true,"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/comments?post=30"}],"version-history":[{"count":25,"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/pages\/30\/revisions"}],"predecessor-version":[{"id":1079,"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/pages\/30\/revisions\/1079"}],"wp:attachment":[{"href":"https:\/\/auditore.cab.inta-csic.es\/masivas-torrejon\/wp-json\/wp\/v2\/media?parent=30"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}