{"id":1677,"date":"2024-08-04T21:23:59","date_gmt":"2024-08-04T21:23:59","guid":{"rendered":"https:\/\/nucleomilenioeris.cl\/?p=1677"},"modified":"2024-08-04T21:24:01","modified_gmt":"2024-08-04T21:24:01","slug":"nuevos-hallazgos-en-la-investigacion-de-la-via-lactea-y-galaxias-asociadas","status":"publish","type":"post","link":"https:\/\/nucleomilenioeris.cl\/es\/news\/nuevos-hallazgos-en-la-investigacion-de-la-via-lactea-y-galaxias-asociadas\/","title":{"rendered":"Nuevos hallazgos en la investigaci\u00f3n de la V\u00eda L\u00e1ctea y Galaxias Asociadas"},"content":{"rendered":"<p>En el campo de la astrof\u00edsica, la comprensi\u00f3n de la V\u00eda L\u00e1ctea, sus componentes y su origen sigue evolucionando gracias a investigaciones innovadoras que exploran la qu\u00edmica estelar y las interacciones gal\u00e1cticas. Estos estudios son cruciales para desentra\u00f1ar la compleja historia de nuestra galaxia y comprender mejor&nbsp; las poblaciones estelares que la conforman.&nbsp;<\/p>\n\n\n\n<p>La reciente aceptaci\u00f3n para publicaci\u00f3n de dos investigaciones por parte de miembros del N\u00facleo Milenio ERIS ofrece nuevas perspectivas sobre estos temas, resaltando la importancia de la diversidad qu\u00edmica y los procesos de acumulaci\u00f3n gal\u00e1ctica en la astrof\u00edsica moderna.<\/p>\n\n\n\n<p>El primer estudio, titulado &#8220;<a href=\"https:\/\/arxiv.org\/abs\/2407.18851\"><em>The Accreted Galaxy: An Overview of TESS Metal-Poor Accreted Stars Candidates<\/em><\/a>&#8220;, liderado por Danielle De Brito y aceptado para su publicaci\u00f3n en la revista <em>Astronomy &amp; Astrophysics<\/em>, aborda la identificaci\u00f3n de estrellas que&nbsp; orbitan en sentido contrario al disco de la V\u00eda L\u00e1ctea, indicando su probable origen fuera de nuestra galaxia. Utilizando observaciones del espectr\u00f3grafo MIKE y datos del cat\u00e1logo TESS, el estudio combina astrosismolog\u00eda, espectroscop\u00eda y astrometr\u00eda para examinar las propiedades internas de estas estrellas.&nbsp;<\/p>\n\n\n\n<p>Para Danielle, esta investigaci\u00f3n es sumamente interesante de ejecutar debido a la peculiaridad del trabajo. \u201cEsto es relevante porque es importante caracterizar mejor las limitaciones que tenemos al usar solo informaci\u00f3n espectrosc\u00f3pica, ya que la informaci\u00f3n astros\u00edsmica de estrellas pobres en metales es limitada en cantidad en comparaci\u00f3n con la informaci\u00f3n disponible para estrellas con mayor contenido met\u00e1lico.\u201d, comenta la autora principal de la investigaci\u00f3n.<\/p>\n\n\n\n<p>La astrosismolog\u00eda permite \u201cescuchar\u201d el interior de las estrellas, proporcionando informaci\u00f3n sobre su masa y edad. Este estudio destaca la colaboraci\u00f3n de Clare Worley, quien contribuir\u00e1 al programa de espectroscop\u00eda gracias a una visita que realizar\u00e1 a Chile desde Nueva Zelanda con parte de su equipo de estudiantes durante noviembre, fortaleciendo el avance en este campo de investigaci\u00f3n.<\/p>\n\n\n\n<p>El segundo art\u00edculo, &#8220;<a href=\"https:\/\/arxiv.org\/abs\/2407.18823\"><em>The Chemical Diversity of the Metal-Poor Milky Way<\/em><\/a>&#8220;, examina la diversidad qu\u00edmica de las estrellas antiguas y pobres en metales en la V\u00eda L\u00e1ctea. Este trabajo, liderado por Nicole Buckley, estudiante de doctorado de la University Of Surrey, fue desarrollado en gran parte durante su visita a Chile, donde colabor\u00f3 estrechamente con Rob Yates, colaborador del N\u00facleo. El art\u00edculo, aceptado para su publicaci\u00f3n en la revista <em>Monthly Notices of the Royal Astronomical Society (MNRAS)<\/em>, utiliza datos del cat\u00e1logo GALAH para identificar diez grupos significativos de estrellas en el espacio qu\u00edmico. Buckley descubri\u00f3 que la componente del disco grueso de la V\u00eda L\u00e1ctea est\u00e1 representada por varios grupos qu\u00edmicos distintos, lo que sugiere una historia m\u00e1s compleja de esta componente de lo que se pensaba previamente. La investigaci\u00f3n de Nicole se dise\u00f1\u00f3 en gran medida durante su estancia en la Universidad Diego Portales, con la supervisi\u00f3n parcial de Payel Das.<\/p>\n\n\n\n<p>Ambos estudios reflejan la importancia de la investigaci\u00f3n colaborativa y la integraci\u00f3n de diversas t\u00e9cnicas en la astrof\u00edsica. La investigaci\u00f3n sobre la diversidad qu\u00edmica y las estrellas acretadas aporta nuevas perspectivas sobre la formaci\u00f3n y evoluci\u00f3n de la V\u00eda L\u00e1ctea, as\u00ed como sobre las galaxias que han interactuado con ella. Estos avances subrayan la continua necesidad de explorar y entender los componentes y procesos que configuran nuestro universo.<\/p>","protected":false},"excerpt":{"rendered":"<p>En el campo de la astrof\u00edsica, la comprensi\u00f3n de la V\u00eda L\u00e1ctea, sus componentes y su origen sigue evolucionando gracias a investigaciones innovadoras que exploran la qu\u00edmica estelar y las interacciones gal\u00e1cticas. Estos estudios son cruciales para desentra\u00f1ar la compleja historia de nuestra galaxia y comprender mejor&nbsp; las poblaciones estelares que la conforman.&nbsp; La reciente [&hellip;]<\/p>","protected":false},"author":5,"featured_media":1678,"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-1677","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-news"],"yoast_head":"<!-- This site is optimized with the Yoast SEO plugin v23.4 - https:\/\/yoast.com\/wordpress\/plugins\/seo\/ -->\n<title>Nuevos hallazgos en la investigaci\u00f3n de la V\u00eda L\u00e1ctea y Galaxias Asociadas | 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\/nuevos-hallazgos-en-la-investigacion-de-la-via-lactea-y-galaxias-asociadas\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Nuevos hallazgos en la investigaci\u00f3n de la V\u00eda L\u00e1ctea y Galaxias Asociadas | ERIS\" \/>\n<meta property=\"og:description\" content=\"En el campo de la astrof\u00edsica, la comprensi\u00f3n de la V\u00eda L\u00e1ctea, sus componentes y su origen sigue evolucionando gracias a investigaciones innovadoras que exploran la qu\u00edmica estelar y las interacciones gal\u00e1cticas. Estos estudios son cruciales para desentra\u00f1ar la compleja historia de nuestra galaxia y comprender mejor&nbsp; las poblaciones estelares que la conforman.&nbsp; La reciente [&hellip;]\" \/>\n<meta property=\"og:url\" content=\"https:\/\/nucleomilenioeris.cl\/es\/news\/nuevos-hallazgos-en-la-investigacion-de-la-via-lactea-y-galaxias-asociadas\/\" \/>\n<meta property=\"og:site_name\" content=\"ERIS\" \/>\n<meta property=\"article:published_time\" content=\"2024-08-04T21:23:59+00:00\" \/>\n<meta property=\"article:modified_time\" content=\"2024-08-04T21:24:01+00:00\" \/>\n<meta property=\"og:image\" content=\"https:\/\/nucleomilenioeris.cl\/wp-content\/uploads\/2024\/08\/1-scaled.jpg\" \/>\n\t<meta property=\"og:image:width\" content=\"2560\" \/>\n\t<meta property=\"og:image:height\" content=\"640\" \/>\n\t<meta property=\"og:image:type\" content=\"image\/jpeg\" \/>\n<meta name=\"author\" content=\"FernandoGutzAdmin\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" 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