{"id":12567,"date":"2022-06-03T11:09:21","date_gmt":"2022-06-03T09:09:21","guid":{"rendered":"https:\/\/www.mdscc.nasa.gov\/?p=12567"},"modified":"2022-06-13T15:31:14","modified_gmt":"2022-06-13T13:31:14","slug":"nueva-imagen-de-un-agujero-negro-proporcinada-por-chandra-de-la-nasa","status":"publish","type":"post","link":"https:\/\/www.mdscc.nasa.gov\/index.php\/2022\/06\/03\/nueva-imagen-de-un-agujero-negro-proporcinada-por-chandra-de-la-nasa\/","title":{"rendered":"Nueva imagen de un agujero negro proporcinada por Chandra de la NASA"},"content":{"rendered":"\n<p class=\"wp-block-paragraph\">Esta imagen muestra un espectacular conjunto de anillos alrededor de un <a href=\"https:\/\/www.nasa.gov\/black-holeshttps:\/\/www.nasa.gov\/black-holes\">agujero negro<\/a>, capturado con el Observatorio de rayos X <a href=\"https:\/\/chandra.harvard.edu\/about\/\">Chandra de la NASA <\/a>y el Observatorio Neil Gehrels Swift. Las im\u00e1genes de rayos X de los gigantes anillos proporcionan informaci\u00f3n sobre el polvo ubicado en nuestra galaxia, utilizando un principio similar a los rayos X realizados en consultorios m\u00e9dicos y aeropuertos.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\">El agujero negro es parte de un sistema binario llamado V404 Cygni, ubicado a casi 8.000 <a href=\"https:\/\/chandra.harvard.edu\/photo\/cosmic_distance.html\">a\u00f1os luz<\/a> de la Tierra. El agujero negro est\u00e1 alejando activamente el material de una estrella compa\u00f1era (que tiene, aproximadamente, la mitad de la masa del Sol) en un disco alrededor del objeto invisible. Este material brilla en rayos X, por lo que los astr\u00f3nomos se refieren a estos sistemas como \u00abbinarios de rayos X\u00bb.<\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><strong><a href=\"https:\/\/www.nasa.gov\/image-feature\/huge-rings-around-a-black-hole\">Noticia original (en ingl\u00e9s)<\/a><\/strong><\/p>\n\n\n\n<p class=\"wp-block-paragraph\"><em>Edici\u00f3n: R. Castro.<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Cr\u00e9ditos:<br \/>\nrayos X: NASA\/CXC\/U.Wisc-Madison\/S. Heinz et al.; \u00d3ptico\/IR: Pan-STARR.<\/p>\n","protected":false},"author":2,"featured_media":12568,"comment_status":"closed","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[79,252],"tags":[],"class_list":["post-12567","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-noticias","category-ultimas-noticias"],"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12567","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/comments?post=12567"}],"version-history":[{"count":3,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12567\/revisions"}],"predecessor-version":[{"id":12603,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/posts\/12567\/revisions\/12603"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/media\/12568"}],"wp:attachment":[{"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/media?parent=12567"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/categories?post=12567"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.mdscc.nasa.gov\/index.php\/wp-json\/wp\/v2\/tags?post=12567"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}