{"id":6416,"date":"2023-06-06T22:00:00","date_gmt":"2023-06-06T22:00:00","guid":{"rendered":"https:\/\/modernsciences.org\/staging\/4414\/?p=6416"},"modified":"2023-05-28T16:14:46","modified_gmt":"2023-05-28T16:14:46","slug":"astronomers-detected-two-major-targets-with-a-single-telescope-a-mysterious-signal-and-its-source-galaxy","status":"publish","type":"post","link":"https:\/\/modernsciences.org\/staging\/4414\/astronomers-detected-two-major-targets-with-a-single-telescope-a-mysterious-signal-and-its-source-galaxy\/","title":{"rendered":"Astronomers detected two major targets with a single telescope \u2013 a mysterious signal and its source galaxy"},"content":{"rendered":"\n  <figure>\n    <img  decoding=\"async\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/521206\/original\/file-20230417-28-c0lcs2.jpg?ixlib=rb-1.1.0&#038;q=45&#038;auto=format&#038;w=754&#038;fit=clip\" >\n      <figcaption>\n        ASKAP multiple landscape backview.\n        <span class=\"attribution\"><span class=\"source\">CSIRO<\/span><\/span>\n      <\/figcaption>\n  <\/figure>\n\n<span><a href=\"https:\/\/theconversation.com\/profiles\/marcin-glowacki-1424297\" target=\"_blank\" rel=\"noopener\">Marcin Glowacki<\/a>, <em><a href=\"https:\/\/theconversation.com\/institutions\/curtin-university-873\" target=\"_blank\" rel=\"noopener\">Curtin University<\/a><\/em><\/span>\n\n<p>Astronomers have been working to better understand the galactic environments of fast radio bursts (FRBs) \u2013 intense, momentary bursts of energy occurring in mere milliseconds and with unknown cosmic origins.<\/p>\n\n<p>Now, a study of the slow-moving, star-forming gas in the same galaxy found to host an FRB <a href=\"https:\/\/doi.org\/10.3847\/1538-4357\/acc1e3\" target=\"_blank\" rel=\"noopener\">has been published in The Astrophysical Journal<\/a>. This is only the fourth-ever publication on two completely different areas of astronomy describing the same galaxy. <\/p>\n\n<p>Even more remarkable is the fact that a single telescope made the discovery possible \u2013 from the same observation. <\/p>\n\n<h2 id=\"fast-radio-mysteries\">Fast radio mysteries<\/h2>\n\n<p>FRBs, first detected in 2007, are incredibly powerful pulses of radio waves. They originate from distant galaxies, and the signal typically only lasts a few milliseconds.<\/p>\n\n<p>FRBs are immensely useful for studying the cosmos, from investigating <a href=\"https:\/\/news.ucsc.edu\/2020\/05\/missing-matter.html\" target=\"_blank\" rel=\"noopener\">the matter that makes up the universe<\/a>, to even using them <a href=\"https:\/\/academic.oup.com\/mnras\/article-abstract\/516\/4\/4862\/6694260\" target=\"_blank\" rel=\"noopener\">to constrain the Hubble constant<\/a> \u2013 the measure of how much the universe is expanding.<\/p>\n\n\n\n<p>However, the origin of FRBs is an ongoing puzzle for astronomers. Some FRBs are known to repeat, <a href=\"https:\/\/iopscience.iop.org\/article\/10.1088\/1674-1056\/aca7ed\" target=\"_blank\" rel=\"noopener\">sometimes over a thousand times<\/a>. Others have only been detected once.<\/p>\n\n<p>Whether these repeating or non-repeating signals have formed differently <a href=\"https:\/\/academic.oup.com\/mnras\/article-abstract\/500\/3\/3275\/5944128\" target=\"_blank\" rel=\"noopener\">is currently being investigated by several research groups<\/a>. At one point, we had more theories on how fast radio bursts are made than detections of them.<\/p>\n\n<p>It\u2019s an exciting time to be studying FRBs, as showcased by the recent study <a href=\"https:\/\/theconversation.com\/for-the-first-time-astronomers-have-linked-a-mysterious-fast-radio-burst-with-gravitational-waves-202341\" target=\"_blank\" rel=\"noopener\">associating an FRB with a gravitational wave<\/a>. If that finding holds true, it means at least some FRBs could be created by two neutron stars merging to form a black hole. <\/p>\n\n<p>However, it is hard to pinpoint where exactly fast radio bursts come from. They are extremely bright yet so brief, getting an accurate position is hard for many radio telescopes. Without knowing where precisely these bursts originate, we cannot study the galaxies they are found in. And without knowing the environments FRBs are formed in, we cannot fully solve their mysteries. <\/p>\n\n<p>One telescope in Australia is now helping us figure it out. <\/p>\n\n<figure class=\"align-center \">\n            <img  decoding=\"async\"  alt=\"\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-ls-sizes=\"(min-width: 1466px) 754px, (max-width: 599px) 100vw, (min-width: 600px) 600px, 237px\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;rect=0%2C232%2C5725%2C3181&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"  data-pk-srcset=\"https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=600&amp;h=400&amp;fit=crop&amp;dpr=1 600w, https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=600&amp;h=400&amp;fit=crop&amp;dpr=2 1200w, https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=600&amp;h=400&amp;fit=crop&amp;dpr=3 1800w, https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;h=503&amp;fit=crop&amp;dpr=1 754w, https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=754&amp;h=503&amp;fit=crop&amp;dpr=2 1508w, https:\/\/images.theconversation.com\/files\/521203\/original\/file-20230417-1956-ensh6k.jpg?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=754&amp;h=503&amp;fit=crop&amp;dpr=3 2262w\" >\n            <figcaption>\n              <span class=\"caption\">Some of the ASKAP dishes.<\/span>\n              <span class=\"attribution\"><span class=\"source\">CSIRO (Author provided)<\/span><\/span>\n            <\/figcaption>\n          <\/figure>\n\n<h2 id=\"the-tool-for-the-job\">The tool for the job<\/h2>\n\n<p><a href=\"https:\/\/www.csiro.au\/askap\" target=\"_blank\" rel=\"noopener\">CSIRO\u2019s ASKAP radio telescope<\/a> (Australian Square Kilometre Array Pathfinder), located in the Western Australian desert, is a remarkable instrument. Made up of an array of 36 dishes separated by up to six kilometres, ASKAP can detect FRBs and <a href=\"https:\/\/astronomy.curtin.edu.au\/research\/craft\/\" target=\"_blank\" rel=\"noopener\">pinpoint them to their host galaxies<\/a>. <\/p>\n\n<p>ASKAP can in fact perform its FRB search at the same time as observations for other science surveys. <a href=\"https:\/\/wallaby-survey.org\/\" target=\"_blank\" rel=\"noopener\">One such ASKAP survey<\/a> will map the star-forming gas in galaxies across the Southern sky, helping us understand how galaxies evolve. <\/p>\n\n<p>During a recent observation for this survey, ASKAP also detected a new FRB, and we were able to identify the galaxy it comes from \u2013 a nearby <a href=\"https:\/\/astronomy.swin.edu.au\/cosmos\/S\/spiral+galaxy\" target=\"_blank\" rel=\"noopener\">spiral galaxy<\/a> much like our own Milky Way. <\/p>\n\n<h2 id=\"a-gas-filled-galaxy\">A gas-filled galaxy<\/h2>\n\n<p>ASKAP was able to find the cold neutral hydrogen gas \u2013 the source of star formation \u2013 in this spiral galaxy. As far as FRB host galaxies go, this is already a rare detection of this gas; only three other cases have been published so far. These <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ac4ca8\" target=\"_blank\" rel=\"noopener\">had required follow-up observations<\/a>, or <a href=\"https:\/\/iopscience.iop.org\/article\/10.3847\/2041-8213\/ac2b35\" target=\"_blank\" rel=\"noopener\">relied on other older observations<\/a>, made with different telescopes.<\/p>\n\n<p>Here, ASKAP gave us both the FRB and the gas surrounding it. It is the first simultaneous detection of these rarely overlapping occurrences.<\/p>\n\n<figure class=\"align-center \">\n            <img  decoding=\"async\"  alt=\"\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-ls-sizes=\"(min-width: 1466px) 754px, (max-width: 599px) 100vw, (min-width: 600px) 600px, 237px\"  data-pk-src=\"https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;fit=clip\"  data-pk-srcset=\"https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=600&amp;h=495&amp;fit=crop&amp;dpr=1 600w, https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=600&amp;h=495&amp;fit=crop&amp;dpr=2 1200w, https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=600&amp;h=495&amp;fit=crop&amp;dpr=3 1800w, https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=45&amp;auto=format&amp;w=754&amp;h=622&amp;fit=crop&amp;dpr=1 754w, https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=30&amp;auto=format&amp;w=754&amp;h=622&amp;fit=crop&amp;dpr=2 1508w, https:\/\/images.theconversation.com\/files\/521001\/original\/file-20230414-20-jqg7qh.png?ixlib=rb-1.1.0&amp;q=15&amp;auto=format&amp;w=754&amp;h=622&amp;fit=crop&amp;dpr=3 2262w\" >\n            <figcaption>\n              <span class=\"caption\">ASKAP both found the cold hydrogen gas (white contours) in this spiral galaxy, and pinpointed an FRB near the centre (location given by the red ellipse). Glowacki et al. 2023; ESO and ASKAP.<\/span>\n              \n            <\/figcaption>\n          <\/figure>\n\n<p>Disturbed gas which ASKAP can detect can give us an indication that a galaxy merger recently happened, which tells us about the star forming history of the galaxy. In turn this gives us clues as to what may cause FRBs. <\/p>\n\n<p>The previous studies of the gas surrounding FRBs found fast radio bursts reside in very dynamic systems, suggesting tumultuous galaxy mergers triggered the bursts.<\/p>\n\n<p>For this particular FRB, however, the host galaxy environment is surprisingly calmer. Further studies will be needed to find out if overall we see disturbed gas environments for FRBs, or if there are distinct scenarios \u2013 and potentially multiple creation paths \u2013 for FRBs.<\/p>\n\n<h2 id=\"more-to-come\">More to come<\/h2>\n\n<p>Given the uniqueness of such dual detections, this result showcases the strength and versatility of ASKAP. This is the first simultaneous detection of both an FRB and the gas in its host galaxy. <\/p>\n\n<p>And this is just the start. ASKAP is set to detect and localise <a href=\"https:\/\/www.atnf.csiro.au\/research\/interferometry\/public\/How_CRACO_works.pdf\" target=\"_blank\" rel=\"noopener\">over a hundred FRBs a year<\/a>. By continuing to work collaboratively with each other, different survey groups will be able to untangle the mysteries behind FRBs, how they form, and their host galaxy environments. <\/p>\n\n<hr>\n\n<p><em>CSIRO acknowledges the Wajarri Yamaji as the Traditional Owners and native title holders of the Inyarrimanha Ilgari Bundara, our Murchison Radio-astronomy Observatory site, where ASKAP is located.<\/em><!-- Below is The Conversation's page counter tag. Please DO NOT REMOVE. --><img  loading=\"lazy\"  decoding=\"async\"  src=\"data:image\/png;base64,iVBORw0KGgoAAAANSUhEUgAAAAEAAAABAQMAAAAl21bKAAAAA1BMVEUAAP+KeNJXAAAAAXRSTlMAQObYZgAAAAlwSFlzAAAOxAAADsQBlSsOGwAAAApJREFUCNdjYAAAAAIAAeIhvDMAAAAASUVORK5CYII=\"  alt=\"The Conversation\"  width=\"1\"  height=\"1\"  style=\"border: none !important; box-shadow: none !important; margin: 0 !important; max-height: 1px !important; max-width: 1px !important; min-height: 1px !important; min-width: 1px !important; opacity: 0 !important; outline: none !important; padding: 0 !important\"  referrerpolicy=\"no-referrer-when-downgrade\"  class=\" pk-lazyload\"  data-pk-sizes=\"auto\"  data-pk-src=\"https:\/\/counter.theconversation.com\/content\/203557\/count.gif?distributor=republish-lightbox-basic\" ><!-- End of code. If you don't see any code above, please get new code from the Advanced tab after you click the republish button. The page counter does not collect any personal data. More info: https:\/\/theconversation.com\/republishing-guidelines --><\/p>\n\n<p><span><a href=\"https:\/\/theconversation.com\/profiles\/marcin-glowacki-1424297\" target=\"_blank\" rel=\"noopener\">Marcin Glowacki<\/a>, Research Associate, <em><a href=\"https:\/\/theconversation.com\/institutions\/curtin-university-873\" target=\"_blank\" rel=\"noopener\">Curtin University<\/a><\/em><\/span><\/p>\n\n<p>This article is republished from <a href=\"https:\/\/theconversation.com\" target=\"_blank\" rel=\"noopener\">The Conversation<\/a> under a Creative Commons license. Read the <a href=\"https:\/\/theconversation.com\/astronomers-detected-two-major-targets-with-a-single-telescope-a-mysterious-signal-and-its-source-galaxy-203557\" target=\"_blank\" rel=\"noopener\">original article<\/a>.<\/p>\n\n","protected":false},"excerpt":{"rendered":"ASKAP multiple landscape backview. CSIRO Marcin Glowacki, Curtin University Astronomers have been working to better understand the galactic&hellip;\n","protected":false},"author":482,"featured_media":6396,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"nf_dc_page":"","fifu_image_url":"","fifu_image_alt":"","footnotes":""},"categories":[14],"tags":[781,782,225,474],"class_list":{"0":"post-6416","1":"post","2":"type-post","3":"status-publish","4":"format-standard","5":"has-post-thumbnail","7":"category-space","8":"tag-fast-radio-burst","9":"tag-frb","10":"tag-galaxy","11":"tag-the-conversation","12":"cs-entry","13":"cs-video-wrap"},"aioseo_notices":[],"_links":{"self":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/6416","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/users\/482"}],"replies":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/comments?post=6416"}],"version-history":[{"count":1,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/6416\/revisions"}],"predecessor-version":[{"id":6417,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/posts\/6416\/revisions\/6417"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/media\/6396"}],"wp:attachment":[{"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/media?parent=6416"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/categories?post=6416"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/modernsciences.org\/staging\/4414\/wp-json\/wp\/v2\/tags?post=6416"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}