{"id":8441,"date":"2022-06-08T18:36:44","date_gmt":"2022-06-08T22:36:44","guid":{"rendered":"https:\/\/spaceandplanetarynewswire.com\/?p=8441"},"modified":"2022-06-08T18:36:44","modified_gmt":"2022-06-08T22:36:44","slug":"rapid-fire-fast-radio-burst-shows-hot-space-between-galaxies","status":"publish","type":"post","link":"https:\/\/spaceandplanetarynewswire.com\/?p=8441","title":{"rendered":"Rapid-Fire Fast Radio Burst Shows Hot Space Between Galaxies"},"content":{"rendered":"<figure style=\"width: 1140px\" class=\"wp-caption alignnone\"><img decoding=\"async\" class=\"size-medium lazyload\" data-src=\"https:\/\/news.cornell.edu\/sites\/default\/files\/styles\/story_thumbnail_xlarge\/public\/0608_fast_0.jpg?itok=boZvSA2U\" width=\"1140\" height=\"641\" src=\"data:image\/svg+xml;base64,PHN2ZyB3aWR0aD0iMSIgaGVpZ2h0PSIxIiB4bWxucz0iaHR0cDovL3d3dy53My5vcmcvMjAwMC9zdmciPjwvc3ZnPg==\" style=\"--smush-placeholder-width: 1140px; --smush-placeholder-aspect-ratio: 1140\/641;\"><figcaption class=\"wp-caption-text\">The Five-hundred-meter Aperture Spherical radio Telescope, known as FAST, in Ghizou province, southwest China, where Fast Radio Burst 20190520B was discovered, is considered the spiritual successor to the now-defunct, Cornell-built Arecibo Observatory in Puerto Rico.<\/figcaption><\/figure>\n<p>A recently discovered, rare and persistent rapid-fire fast radio burst source \u2013 sending out an occasional and informative cosmic ping from more than 3.5 billion light years away \u2013 helps to reveal the secrets of the broiling hot space between the galaxies. That\u2019s according to an international team of astronomers who published their&nbsp;<a href=\"https:\/\/www.nature.com\/articles\/s41586-022-04755-5\">findings<\/a>&nbsp;in the journal&nbsp;<em>Nature<\/em>.<\/p>\n<p>Fast Radio Burst 20190520B \u2013 a prolific repeating burst source&nbsp;\u2013 was first observed in June 2019 by the Five-hundred-meter Aperture Spherical radio Telescope (FAST), in Ghizou province, southwest China. Astronomers generally consider this telescope as the spiritual successor to the now-defunct, Cornell University-built Arecibo Observatory in Puerto Rico.<\/p>\n<p>After FAST found the burst, scientists then pinpointed the burst\u2019s location using the Very Large Array, Socorro, New Mexico.<\/p>\n<p>What excites astronomers about the repeating fast radio bursts (FRBs) \u2013 since they only burst once, generally speaking \u2013 is that these quick-fire surges provide a pathway for scientists to comprehend the perplexing, mysterious and million-degree intergalactic medium.<\/p>\n<p>\u201cExamining the intergalactic medium is really hard,\u201d said co-author Shami Chatterjee, principal research scientist in astronomy at Cornell. \u201cThe intergalactic medium is difficult to probe, which is why fast radio bursts are exciting. The bursts let us study the properties of the intergalactic medium.\u201d<\/p>\n<p>Joining Chatterjee on the Nature paper are James M. Cordes, professor of astronomy and Stella K. Ocker, a doctoral student in astronomy.<\/p>\n<p>Co-author Di Li, is the chief scientist of both FAST and the radio division of the National Astronomical Observatories of Chinese Academy of Sciences. The observatory has discovered more than 100 pulsars and more than 5 FRBs.<\/p>\n<p>Four bursts were detected during the initial 24-second scan in 2019, according to the paper. Between April and September 2020, during follow-up observations, FAST detected 75.<\/p>\n<p>Due to the rapidly repeating bursts, astronomers believe that FRB 20190520B may be quite young. \u201cIt seems to reside in a complex plasma environment, like that expected in a young supernova remnant,\u201d Chatterjee said. \u201cSo one possibility is that the highly active source may be a newborn, and if so, it paints an intriguing evolutionary picture of FRB sources, where young burst sources are associated with persistent radio emission.<\/p>\n<p>\u201cThe persistent emission fades away as the burst repetition rate slows down,\u201d Chatterjee said. \u201cThis is still very much a hypothesis and we are eager to test it with further examples of repeating FRBs.\u201d<\/p>\n<p>Astronomers usually assume that FRBs pass through only a modest amount of gas (free electrons) in their host galaxies, which makes counting electrons in the intergalactic medium an easier task. FRB 20190520B shows the opposite: It has encountered far more gas in its host galaxy than scientists expected, calling into question previous assumptions.<\/p>\n<p>Ultimately, astronomers want to know how the intergalactic medium is formed.<\/p>\n<p>\u201cWe want to deconstruct how many free electrons are in the intergalactic medium, because it has been extremely difficult to study,\u201d Ocker said. \u201cWe don\u2019t know much about it.\u201d<\/p>\n<p>\u201cThis particular new repeating FRB behaves in extreme, surprising ways,\u201d Ocker said.<\/p>\n","protected":false},"excerpt":{"rendered":"<p>A recently discovered, rare and persistent rapid-fire fast radio burst source \u2013 sending out an occasional and informative cosmic ping from more than 3.5 billion light years away \u2013 helps to reveal the secrets of the broiling hot space between the galaxies. That\u2019s according to an international team of astronomers who published their&nbsp;findings&nbsp;in the journal&nbsp;Nature.&hellip;<\/p>\n","protected":false},"author":71,"featured_media":8443,"comment_status":"open","ping_status":"closed","sticky":false,"template":"","format":"standard","meta":{"ngg_post_thumbnail":0,"fifu_image_url":"https:\/\/news.cornell.edu\/sites\/default\/files\/styles\/story_thumbnail_xlarge\/public\/0608_fast_0.jpg?itok=boZvSA2U","fifu_image_alt":"Rapid-Fire Fast Radio Burst Shows Hot Space Between Galaxies","footnotes":""},"categories":[216],"tags":[],"class_list":["post-8441","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-discovery"],"_links":{"self":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8441","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/users\/71"}],"replies":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcomments&post=8441"}],"version-history":[{"count":1,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8441\/revisions"}],"predecessor-version":[{"id":8442,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/posts\/8441\/revisions\/8442"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=\/wp\/v2\/media\/8443"}],"wp:attachment":[{"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fmedia&parent=8441"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Fcategories&post=8441"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/spaceandplanetarynewswire.com\/index.php?rest_route=%2Fwp%2Fv2%2Ftags&post=8441"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}