{"id":39,"date":"2016-01-03T22:19:02","date_gmt":"2016-01-03T22:19:02","guid":{"rendered":"http:\/\/wdb.ugr.es\/~fqm292\/wordpress\/?page_id=39"},"modified":"2023-02-21T16:12:51","modified_gmt":"2023-02-21T16:12:51","slug":"research","status":"publish","type":"page","link":"https:\/\/wpd.ugr.es\/~fqm292\/research\/","title":{"rendered":"Research"},"content":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; admin_label=&#8221;section&#8221; _builder_version=&#8221;3.22&#8243;][et_pb_row admin_label=&#8221;row&#8221; _builder_version=&#8221;3.25&#8243; background_size=&#8221;initial&#8221; background_position=&#8221;top_left&#8221; background_repeat=&#8221;repeat&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;3.25&#8243; custom_padding=&#8221;|||&#8221; custom_padding__hover=&#8221;|||&#8221;][et_pb_text admin_label=&#8221;Research&#8221; _builder_version=&#8221;3.27.4&#8243; text_text_color=&#8221;#666666&#8243; background_size=&#8221;initial&#8221; background_position=&#8221;top_left&#8221; background_repeat=&#8221;repeat&#8221; use_border_color=&#8221;off&#8221;]<\/p>\n<h2>Areas of interest<\/h2>\n<ul>\n<li>Chemical Composition of Cool Stars<\/li>\n<li>Structure and Evolution of Low and Intermediate Mass Stars<\/li>\n<li>High Resolution Stellar Spectroscopy<\/li>\n<li>AGB Stars<\/li>\n<li>Nucleosynthesis<\/li>\n<li>Thermonuclear Supernovae: Progenitors, Explosions and Cosmology<\/li>\n<li>Chemical Evolution of the Universe<\/li>\n<li>Asteroseismology from the space<\/li>\n<li>Detection and characterization of extrasolar planets<\/li>\n<li>Astroparticles<\/li>\n<li>SN host Galaxies and their properties<\/li>\n<li>SPH hydrodynamical simulations of colliding stars<\/li>\n<\/ul>\n<h2><\/h2>\n<h2>Current Projects<\/h2>\n<ul>\n<li>PID2021-123110NB-I00. <em>Las estrellas de masa baja e intermedia como motores de la evoluci\u00f3n qu\u00edmica, progenitores de supernova y laboratorio de astropart\u00edculas<\/em> III. 2022-2026, 84,000 \u20ac.<\/li>\n<li>PID2019-107061GB-C64. <em>Contribuci\u00f3n de la UGR a la misi\u00f3n espacial PLATO2.0.<\/em> Fases C\/D-1. 2020-2024, 277,211 \u20ac.<\/li>\n<li>E\u2010FQM\u2010041\u2010UGR18. <em>Caracterizaci\u00f3n de estrellas rotantes.<\/em> 2020-2023<em>, <\/em>141,150 \u20ac.<\/li>\n<\/ul>\n<p>[\/et_pb_text][\/et_pb_column][\/et_pb_row][\/et_pb_section]<\/p>\n","protected":false},"excerpt":{"rendered":"<p>[et_pb_section fb_built=&#8221;1&#8243; admin_label=&#8221;section&#8221; _builder_version=&#8221;3.22&#8243;][et_pb_row admin_label=&#8221;row&#8221; _builder_version=&#8221;3.25&#8243; background_size=&#8221;initial&#8221; background_position=&#8221;top_left&#8221; background_repeat=&#8221;repeat&#8221;][et_pb_column type=&#8221;4_4&#8243; _builder_version=&#8221;3.25&#8243; custom_padding=&#8221;|||&#8221; custom_padding__hover=&#8221;|||&#8221;][et_pb_text admin_label=&#8221;Research&#8221; _builder_version=&#8221;3.27.4&#8243; text_text_color=&#8221;#666666&#8243; background_size=&#8221;initial&#8221; background_position=&#8221;top_left&#8221; background_repeat=&#8221;repeat&#8221; use_border_color=&#8221;off&#8221;] Areas of interest Chemical Composition of Cool Stars Structure and Evolution of Low and Intermediate Mass Stars High Resolution Stellar Spectroscopy AGB Stars Nucleosynthesis Thermonuclear Supernovae: Progenitors, Explosions and Cosmology Chemical Evolution of the Universe [&hellip;]<\/p>\n","protected":false},"author":1,"featured_media":0,"parent":0,"menu_order":0,"comment_status":"closed","ping_status":"closed","template":"","meta":{"_et_pb_use_builder":"on","_et_pb_old_content":"","_et_gb_content_width":""},"_links":{"self":[{"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/pages\/39"}],"collection":[{"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/pages"}],"about":[{"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/types\/page"}],"author":[{"embeddable":true,"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/users\/1"}],"replies":[{"embeddable":true,"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/comments?post=39"}],"version-history":[{"count":22,"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/pages\/39\/revisions"}],"predecessor-version":[{"id":1001,"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/pages\/39\/revisions\/1001"}],"wp:attachment":[{"href":"https:\/\/wpd.ugr.es\/~fqm292\/wp-json\/wp\/v2\/media?parent=39"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}