{"id":1674,"date":"2024-08-04T21:22:09","date_gmt":"2024-08-04T21:22:09","guid":{"rendered":"https:\/\/nucleomilenioeris.cl\/?p=1674"},"modified":"2024-08-04T21:22:16","modified_gmt":"2024-08-04T21:22:16","slug":"avances-en-la-calibracion-de-lineas-de-absorcion-usando-cefeidas-clasicas","status":"publish","type":"post","link":"https:\/\/nucleomilenioeris.cl\/es\/news\/avances-en-la-calibracion-de-lineas-de-absorcion-usando-cefeidas-clasicas\/","title":{"rendered":"Avances en la calibraci\u00f3n de L\u00edneas de Absorci\u00f3n usando Cefeidas Cl\u00e1sicas"},"content":{"rendered":"

Miembro del N\u00facleo Milenio ERIS, ha logrado la aceptaci\u00f3n de su paper titulado “Astrophysical calibration of the oscillator strengths of YJ-band absorption lines in classical Cepheids<\/em><\/a>” en la revista Monthly Notices of the Royal Astronomical Society (MNRAS)<\/em>. Este trabajo se deriva de su investigaci\u00f3n doctoral en Tokio y tiene implicaciones directas en los proyectos actuales de ERIS.<\/p>\n\n\n\n

El paper presenta un an\u00e1lisis de bandas infrarrojas (Y y J) en estrellas variables Cefeidas. Estas estrellas son conocidas por sus cambios peri\u00f3dicos en tama\u00f1o y luminosidad, lo que las hace \u00fatiles para la escala de distancias gal\u00e1ctica y extragal\u00e1ctica. Adem\u00e1s, sus espectros muestran una variedad de elementos qu\u00edmicos en sus l\u00edneas de absorci\u00f3n. Scarlet Sandoval, autora de la investigaci\u00f3n explica que “la probabilidad de que un electr\u00f3n de un \u00e1tomo o ion absorba un fot\u00f3n de una longitud de onda en particular y experimente una ‘transici\u00f3n’ de un estado de energ\u00eda m\u00e1s bajo a uno m\u00e1s alto” se cuantifica mediante la fuerza del oscilador, conocida como “oscillator strengths”.<\/p>\n\n\n\n

Para caracterizar una l\u00ednea de absorci\u00f3n, es esencial conocer cantidades at\u00f3micas como el oscilador, el potencial de excitaci\u00f3n y los coeficientes de van der Waals. Estos datos, generalmente obtenidos te\u00f3ricamente por la mec\u00e1nica cu\u00e1ntica y verificados en laboratorios, se prueban en observaciones reales de estrellas. S. Elgueta se\u00f1ala que “el estudio de los elementos qu\u00edmicos y mol\u00e9culas presentes en las estrellas se ha hecho mayoritariamente en bandas \u00f3pticas, pero pocas veces en bandas infrarrojas”.<\/p>\n\n\n\n

Utilizando el espectr\u00f3grafo WINERED, Sandoval explor\u00f3 las bandas del infrarrojo cercano (Y-J) y descubri\u00f3 una abundancia de elementos y mol\u00e9culas poco estudiadas. Este trabajo result\u00f3 en la creaci\u00f3n de un atlas de l\u00edneas y constantes at\u00f3micas calibradas para objetos en reg\u00edmenes m\u00e1s calientes, como las Cefeidas cl\u00e1sicas. La informaci\u00f3n obtenida ayuda a entender fen\u00f3menos de la arqueolog\u00eda gal\u00e1ctica, como el gradiente de metalicidad de la V\u00eda L\u00e1ctea y la producci\u00f3n de elementos pesados.<\/p>\n\n\n\n

Este paper tambi\u00e9n es fundamental para el proyecto actual de S. Elgueta en ERIS, en colaboraci\u00f3n con la Dra. Paula Jofr\u00e9 y la Dra. Ulrike Heiter. En este proyecto, se caracteriza la muestra de Gaia Benchmark Stars observadas en todo el infrarrojo con el espectr\u00f3grafo CRIRES+. La autora de la investigaci\u00f3n finaliza mencionando que “esto supondr\u00e1 un nuevo atlas mucho m\u00e1s completo y optimizado para cualquier usuario cuya muestra se asocie de una u otra forma a alguna de las representantes de nuestras GBS”.<\/p>","protected":false},"excerpt":{"rendered":"

Miembro del N\u00facleo Milenio ERIS, ha logrado la aceptaci\u00f3n de su paper titulado “Astrophysical calibration of the oscillator strengths of YJ-band absorption lines in classical Cepheids” en la revista Monthly Notices of the Royal Astronomical Society (MNRAS). Este trabajo se deriva de su investigaci\u00f3n doctoral en Tokio y tiene implicaciones directas en los proyectos actuales […]<\/p>","protected":false},"author":5,"featured_media":1675,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"site-sidebar-layout":"default","site-content-layout":"","ast-site-content-layout":"default","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":"set","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 center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"ast-content-background-meta":{"desktop":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"tablet":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""},"mobile":{"background-color":"var(--ast-global-color-5)","background-image":"","background-repeat":"repeat","background-position":"center center","background-size":"auto","background-attachment":"scroll","background-type":"","background-media":"","overlay-type":"","overlay-color":"","overlay-opacity":"","overlay-gradient":""}},"footnotes":""},"categories":[6],"tags":[],"class_list":["post-1674","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"yoast_head":"\nAvances en la calibraci\u00f3n de L\u00edneas de Absorci\u00f3n usando Cefeidas Cl\u00e1sicas | ERIS<\/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:\/\/nucleomilenioeris.cl\/es\/news\/avances-en-la-calibracion-de-lineas-de-absorcion-usando-cefeidas-clasicas\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Avances en la calibraci\u00f3n de L\u00edneas de Absorci\u00f3n usando Cefeidas Cl\u00e1sicas | ERIS\" \/>\n<meta property=\"og:description\" content=\"Miembro del N\u00facleo Milenio ERIS, ha logrado la aceptaci\u00f3n de su paper titulado “Astrophysical calibration of the oscillator strengths of YJ-band absorption lines in classical Cepheids” en la revista Monthly Notices of the Royal Astronomical Society (MNRAS). 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