{"id":186540,"date":"2025-10-31T10:28:30","date_gmt":"2025-10-31T09:28:30","guid":{"rendered":"https:\/\/helloproject.es\/vigilancia\/una-nebulosa-con-forma-de-murcielago-revela-una-activa-region-de-formacion-estelar\/"},"modified":"2025-10-31T10:28:30","modified_gmt":"2025-10-31T09:28:30","slug":"una-nebulosa-con-forma-de-murcielago-revela-una-activa-region-de-formacion-estelar","status":"publish","type":"post","link":"https:\/\/helloproject.es\/vigilancia\/una-nebulosa-con-forma-de-murcielago-revela-una-activa-region-de-formacion-estelar\/","title":{"rendered":"Una nebulosa con forma de murci\u00e9lago revela una activa regi\u00f3n de formaci\u00f3n estelar"},"content":{"rendered":"

Una nube c\u00f3smica de gran tama\u00f1o ha sido captada por el telescopio VLT Survey Telescope (VST) del Observatorio Europeo Austral (ESO), ubicado en el desierto de Atacama, Chile. La imagen muestra una nebulosa cuya silueta recuerda a la de un murci\u00e9lago con las alas extendidas, enmarcada por un cielo estrellado. Esta formaci\u00f3n se encuentra entre las constelaciones australes de Circinus y Norma, y ocupa una regi\u00f3n del cielo equivalente a cuatro lunas llenas.<\/p>\n

La formaci\u00f3n se encuentra entre las constelaciones australes de Circinus y Norma, y ocupa una regi\u00f3n del cielo equivalente a cuatro lunas llenas<\/p>\n

La nebulosa, situada a unos 10 000 a\u00f1os luz de distancia, es una regi\u00f3n de formaci\u00f3n estelar activa. En su interior, las estrellas j\u00f3venes emiten suficiente energ\u00eda para excitar los \u00e1tomos de hidr\u00f3geno circundantes, lo que genera el caracter\u00edstico resplandor rojo visible en la imagen. Las zonas oscuras que atraviesan la nube corresponden a filamentos de gas m\u00e1s fr\u00edo y denso, con part\u00edculas de polvo que bloquean la luz de las estrellas situadas detr\u00e1s.<\/p>\n

<\/a><\/p>\n

Regiones brillantes de formaci\u00f3n estelar<\/h2>\n

Los componentes m\u00e1s destacados de esta estructura son RCW 94, que forma el ala derecha, y RCW 95, que constituye el cuerpo. Ambos pertenecen a un cat\u00e1logo de regiones brillantes de formaci\u00f3n estelar en el cielo austral. El resto de la figura no cuenta con una designaci\u00f3n oficial.<\/p>\n

La imagen fue obtenida con la c\u00e1mara OmegaCAM de 268 megap\u00edxeles instalada en el VST, operado por el Instituto Nacional de Astrof\u00edsica de Italia<\/p>\n

La imagen fue obtenida gracias a OmegaCAM, una c\u00e1mara de 268 megap\u00edxeles instalada en el VST, operado por el Instituto Nacional de Astrof\u00edsica de Italia (INAF).<\/p>\n

Esta c\u00e1mara permite capturar amplias zonas del cielo con gran detalle. Para construir la imagen, se combinaron observaciones en diferentes longitudes de onda. La mayor parte del contorno y el brillo rojo fueron registrados en luz visible como parte del proyecto VPHAS+, mientras que los datos infrarrojos, obtenidos con el telescopio VISTA, aportan informaci\u00f3n adicional sobre las zonas m\u00e1s densas de la nebulosa. Ambos estudios est\u00e1n disponibles para el p\u00fablico interesado en explorar el universo a trav\u00e9s de im\u00e1genes astron\u00f3micas.<\/p>","protected":false},"excerpt":{"rendered":"

Una nube c\u00f3smica de gran tama\u00f1o ha sido captada por el telescopio VLT Survey Telescope (VST) del Observatorio Europeo Austral (ESO), ubicado en el desierto de Atacama, Chile. La imagen muestra una nebulosa cuya silueta recuerda a la de un murci\u00e9lago con las alas extendidas, enmarcada por un cielo estrellado. Esta formaci\u00f3n se encuentra entre […]<\/p>\n","protected":false},"author":5,"featured_media":0,"comment_status":"","ping_status":"","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":"","ast-disable-related-posts":"","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":"default","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":[5],"tags":[],"class_list":["post-186540","post","type-post","status-publish","format-standard","hentry","category-noticias"],"yoast_head":"\nUna nebulosa con forma de murci\u00e9lago revela una activa regi\u00f3n de formaci\u00f3n estelar - bip4ex<\/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:\/\/helloproject.es\/vigilancia\/una-nebulosa-con-forma-de-murcielago-revela-una-activa-region-de-formacion-estelar\/\" \/>\n<meta property=\"og:locale\" content=\"es_ES\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Una nebulosa con forma de murci\u00e9lago revela una activa regi\u00f3n de formaci\u00f3n estelar\" \/>\n<meta property=\"og:description\" content=\"Una nube c\u00f3smica de gran tama\u00f1o ha sido captada por el telescopio VLT Survey Telescope (VST) del Observatorio Europeo Austral (ESO), ubicado en el desierto de Atacama, Chile. 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