{"id":7877,"date":"2016-02-28T04:17:12","date_gmt":"2016-02-28T04:17:12","guid":{"rendered":"http:\/\/revoscience.com\/en\/?p=7877"},"modified":"2016-02-28T04:17:12","modified_gmt":"2016-02-28T04:17:12","slug":"mysterious-cosmic-radio-bursts-found-to-repeat","status":"publish","type":"post","link":"https:\/\/www.revoscience.com\/en\/mysterious-cosmic-radio-bursts-found-to-repeat\/","title":{"rendered":"Mysterious cosmic radio bursts found to repeat"},"content":{"rendered":"

Astronomers for the first time detect repeat \u2018fast radio bursts\u2019 from same sky location<\/span><\/strong><\/p>\n

Dwingeloo,–\u00a0Astronomers for the first time have detected repeating short-duration bursts of radio waves from an enigmatic source which is likely located well beyond the edge of our Milky Way galaxy. The findings indicate that these \u201cfast radio bursts\u201d come from an extremely powerfu<\/span><\/p>\n

\"Image<\/a>
Image 1: The 305-m Arecibo telescope and its suspended support platform of radio receivers is shown amid a starry night. From space, a sequence of millisecond-duration radio flashes are racing towards the dish, where they will be reflected and detected by the radio receivers. Such radio signals are called fast radio bursts, and Arecibo is the first telescope to see repeat bursts from the same source.
Figure Credit: Danielle Futselaar<\/figcaption><\/figure>\n

l object which occasionally produces multiple bursts in under a minute.<\/span>
\n\u00a0<\/span>
\nPrior to this discovery, reported in Nature, all previously detected fast radio bursts (FRBs) have appeared to be one-off events. Because of that, most theories about the origin of these mysterious pulses have involved cataclysmic incidents that destroy their source \u2013 a star exploding in a supernova, for example, or a neutron star collapsing into a black hole. The new finding, however, shows that at least some FRBs have other origins.<\/span>
\n\u00a0<\/span>
\nFRBs, which last just a few thousandths of a second, have puzzled scientists since they were first reported nearly a decade ago. Despite extensive follow-up efforts, astronomers until now have searched in vain for repeat bursts.<\/span>
\n\u00a0<\/span>
\nThat changed last\u00a0November 5th<\/span>, when McGill University PhD student Paul Scholz was sifting through results from observations performed with the Arecibo radio telescope in Puerto Rico \u2013 the world\u2019s largest radio telescope. The new data showed several bursts with properties consistent with those of an FRB detected in 2012.<\/span>
\n\u00a0<\/span>
\nThe repeat signals were surprising \u2013 and \u201cvery exciting,\u201d Scholz says. \u201cI knew immediately that the discovery would be extremely important in the study of FRBs.\u201d As his office mates gathered around his computer screen, Scholz pored over the remaining output from specialized software used to search for pulsars and radio bursts. He found that there were a total of 10 new bursts.<\/span><\/p>\n

[pullquote]The finding suggests that these bursts must have come from a very exotic object, such as a rotating neutron star having unprecedented power that enables the emission of extremely bright pulses, the researchers say[\/pullquote]
\n\u00a0<\/span>
\nThe finding suggests that these bursts must have come from a very exotic object, such as a rotating neutron star having unprecedented power that enables the emission of extremely bright pulses, the researchers say. \u00a0It is also possible that the finding represents the first discovery of a sub-class of the cosmic fast-radio-burst population.<\/span>
\n\u00a0<\/span>
\n\u201cNot only did these bursts repeat, but their brightness and spectra also differ from those of other FRBs,\u201d notes Laura Spitler, first author of the new paper and a postdoctoral researcher at the Max Planck Institute for Radio Astronomy in Bonn, Germany.<\/span>
\n\u00a0<\/span>
\nScientists believe that these and other radio bursts originate from distant galaxies, based on \u00a0the measurement of an effect known as plasma dispersion. Pulses that travel through the cosmos are distinguished from man-made interference by the influence of interstellar electrons, which cause radio waves to travel more slowly at lower radio frequencies. The 10 newly discovered bursts, like the one detected in 2012, have three times the maximum dispersion measure that would be expected from a source within the Milky Way.<\/span><\/p>\n

\"Image<\/a>
Image 2: The initially discovered \u201cBurst 1\u201d and 10 new bursts seen from the fast radio burst source FRB 121102. The bursts are shown as a function of radio observing frequency, and the signal summed across all observed frequencies is shown at the top in each case. Figure Credit: Paul Scholz (Figure 2 from the Spitler et al. Nature paper).<\/figcaption><\/figure>\n

Intriguingly, the most likely implication of the new Arecibo finding \u2013 that the repeating FRB \u00a0originates from a very young extragalactic neutron star \u2013 is at odds with the results of a study published last week in Nature by another research team. That paper suggested FRBs are related to cataclysmic events, such as short gamma-ray bursts, which cannot generate repeat events. \u00a0However, the apparent conflict between the studies could be resolved, if it turns out that there are at least two kinds of FRB sources.<\/span>
\n\u00a0<\/span>
\nIn future research, the team hopes to identify the galaxy where the radio bursts originated. To do so, they will need to detect bursts using radio telescopes with far more resolving power than Arecibo, a National Science Foundation-sponsored facility with a dish that spans 305 metres and covers about 20 acres. Using a technique called interferometry, performed with radio telescope arrays spread over large geographical distances, the astronomers may be able to achieve the needed resolution.<\/span>
\n\u00a0<\/span>
\n\u201cOnce we have precisely localized the repeater\u2019s position on the sky, we will be able to compare observations from optical and X-ray telescopes and see if there is a galaxy there,\u201d says Jason Hessels, associate professor at the University of Amsterdam and ASTRON, the Netherlands Institute for Radio Astronomy, as well as corresponding author of the Nature paper. \u00a0\u201cFinding the host galaxy of this source is critical to understanding its properties\u201d, he adds.<\/span>
\n\u00a0<\/span>
\nThe Arecibo Observatory is operated by SRI International under a cooperative agreement with the National Science Foundation (AST-1100968), and in alliance with Ana G. M\u00e9ndez-Universidad Metropolitana, and the Universities Space Research Association.<\/span>
\n\u00a0<\/span>
\nThe research was supported by grants from the European Research Council, the National Science and Engineering Council of Canada, and the American National Science Foundation.<\/span><\/p>\n","protected":false},"excerpt":{"rendered":"

Dwingeloo,– Astronomers for the first time have detected repeating short-duration bursts of radio waves from an enigmatic source which is likely located well beyond the edge of our Milky Way galaxy.<\/p>\n","protected":false},"author":2,"featured_media":7878,"comment_status":"open","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"footnotes":""},"categories":[20],"tags":[],"class_list":["post-7877","post","type-post","status-publish","format-standard","has-post-thumbnail","hentry","category-space-news"],"featured_image_urls":{"full":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1-150x150.jpeg",150,150,true],"medium":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1-224x300.jpeg",224,300,true],"medium_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"1536x1536":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"2048x2048":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"ultp_layout_landscape_large":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"ultp_layout_landscape":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"ultp_layout_portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"ultp_layout_square":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"newspaper-x-single-post":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"newspaper-x-recent-post-big":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",270,360,false],"newspaper-x-recent-post-list-image":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",49,65,false],"web-stories-poster-portrait":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",336,448,false],"web-stories-publisher-logo":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",72,96,false],"web-stories-thumbnail":["https:\/\/www.revoscience.com\/en\/wp-content\/uploads\/2016\/02\/Image_1.jpeg",150,200,false]},"author_info":{"info":["RevoScience"]},"category_info":"Space\/ AstroPhysics<\/a>","tag_info":"Space\/ AstroPhysics","comment_count":"0","_links":{"self":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/7877","targetHints":{"allow":["GET"]}}],"collection":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts"}],"about":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/types\/post"}],"author":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/users\/2"}],"replies":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/comments?post=7877"}],"version-history":[{"count":0,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/posts\/7877\/revisions"}],"wp:featuredmedia":[{"embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media\/7878"}],"wp:attachment":[{"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/media?parent=7877"}],"wp:term":[{"taxonomy":"category","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/categories?post=7877"},{"taxonomy":"post_tag","embeddable":true,"href":"https:\/\/www.revoscience.com\/en\/wp-json\/wp\/v2\/tags?post=7877"}],"curies":[{"name":"wp","href":"https:\/\/api.w.org\/{rel}","templated":true}]}}