{"id":32452,"date":"2023-03-24T09:55:39","date_gmt":"2023-03-24T08:55:39","guid":{"rendered":"https:\/\/cab.inta-csic.es\/?post_type=tesis&#038;p=32452"},"modified":"2023-06-15T13:22:06","modified_gmt":"2023-06-15T11:22:06","slug":"astrophysical-parameters-of-m-dwarfs-with-exoplanets","status":"publish","type":"tesis","link":"https:\/\/cab.inta-csic.es\/en\/tesis\/astrophysical-parameters-of-m-dwarfs-with-exoplanets\/","title":{"rendered":"Astrophysical parameters of M dwarfs with exoplanets"},"content":{"rendered":"\n<p>M dwarfs are the most abundant stars in the Universe. They are hosts of a rich diversity of planetary companions, which are much more noticeable in these smaller stars. Advancements in technology continue to push the boundaries of what is possible to be detected on them, even when they exist as faint signals. In many cases, planets orbiting M dwarfs can also be described in remarkable detail. What makes the difference is how deeply we can characterise the host star. This includes to properly model their atmospheres, their abundance of metals, and their activity processes. If they are well described individually, these numerous stars have the potential for providing statistically robust conclusions when combined into larger samples. Carmencita is the input catalogue of nearby M dwarfs for the CARMENES project, which aims to search for potentially habitable Earth-sized planets orbiting them. It contains more than two thousand M dwarfs that are scrutinized by the consortium members from multiple angles and with a high degree of attention to detail.<\/p>\n\n\n\n<div style=\"height:45px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<h5><strong>Par\u00e1metros astrof\u00edsicos de estrellas M con exoplanetas<\/strong><\/h5>\n\n\n\n<div style=\"height:25px\" aria-hidden=\"true\" class=\"wp-block-spacer\"><\/div>\n\n\n\n<p>Las enanas M son las estrellas m\u00e1s abundantes en el Universo. Albergan una rica diversidad de compa\u00f1eros planetarios, que son mucho m\u00e1s evidentes en estas estrellas m\u00e1s peque\u00f1as. Los avances tecnol\u00f3gicos contin\u00faan ampliando los l\u00edmites de lo que es posible detectar en ellas, incluso cuando se manifiestan como se\u00f1ales d\u00e9biles. En muchos casos, los planetas que orbitan enanas M tambi\u00e9n pueden describirse con notable detalle. Lo que marca la diferencia es la completitud con el que podemos caracterizar la estrella anfitriona. Esto incluye modelar adecuadamente sus atm\u00f3sferas, su abundancia en metales y sus procesos de actividad. Si se describen adecuadamente de manera individualizada, estas numerosas estrellas tienen el potencial de proporcionar conclusiones estad\u00edsticamente robustas cuando secombinan en muestras m\u00e1s grandes. Carmencita es el cat\u00e1logo de entrada de enanas M cercanas para el proyecto CARMENES, que tiene como objetivo buscar planetas del tama\u00f1o de la Tierra potencialmente habitables orbitando alrededor de ellas. Contiene m\u00e1s de dos mil enanas M que son examinadas por los miembros del consorcio desde m\u00faltiples \u00e1ngulos y con un alto grado de atenci\u00f3n al detalle.<\/p>\n\n\n\n<p><br><\/p>\n\n\n\n<p><\/p>\n","protected":false},"featured_media":0,"parent":0,"template":"","meta":[],"departamento_global":[492],"tesis_anos":[682],"acf":[],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v20.0 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Astrophysical parameters of M dwarfs with exoplanets &ndash; CAB<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/cab.inta-csic.es\/en\/tesis\/astrophysical-parameters-of-m-dwarfs-with-exoplanets\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Astrophysical parameters of M dwarfs with exoplanets &ndash; CAB\" \/>\n<meta property=\"og:description\" content=\"M dwarfs are the most abundant stars in the Universe. They are hosts of a rich diversity of planetary companions, which are much more noticeable in these smaller stars. Advancements in technology continue to push the boundaries of what is possible to be detected on them, even when they exist as faint signals. 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