  {"id":29606,"date":"2014-11-21T13:50:38","date_gmt":"2014-11-21T23:50:38","guid":{"rendered":"http:\/\/www.hawaii.edu\/news\/?p=29606"},"modified":"2021-10-19T14:46:46","modified_gmt":"2021-10-20T00:46:46","slug":"scientists-use-hawaii-observatories-to-study-an-exotic-object","status":"publish","type":"post","link":"https:\/\/www.hawaii.edu\/news\/2014\/11\/21\/scientists-use-hawaii-observatories-to-study-an-exotic-object\/","title":{"rendered":"Scientists use <span aria-label=\"Hawaii\">Hawai&#699;i<\/span> observatories to study an exotic object"},"content":{"rendered":"<span class=\"span-reading-time rt-reading-time\" style=\"display: block;\"><span class=\"rt-label rt-prefix\">Reading time: <\/span> <span class=\"rt-time\"> 2<\/span> <span class=\"rt-label rt-postfix\">minutes<\/span><\/span><figure id=\"attachment_29630\" aria-describedby=\"caption-attachment-29630\" style=\"width: 300px\" class=\"wp-caption alignright\"><img loading=\"lazy\" decoding=\"async\" src=\"http:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2014\/11\/exotic-object.jpg\" alt=\"\" width=\"300\" height=\"316\" class=\"size-full wp-image-29630\" srcset=\"https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2014\/11\/exotic-object.jpg 300w, https:\/\/www.hawaii.edu\/news\/wp-content\/uploads\/2014\/11\/exotic-object-246x260.jpg 246w\" sizes=\"auto, (max-width: 300px) 100vw, 300px\" \/><figcaption id=\"caption-attachment-29630\" class=\"wp-caption-text\">SDSS1133 (lower left) and Markarian 177. (credit W.M. Keck Observatory.\/M. Koss (ETH Zurich) et al.)<\/figcaption><\/figure>\n<p>An international team of researchers analyzing decades of observations from many facilities, including the <a href=\"http:\/\/www.keckobservatory.org\/\">W.M. Keck Observatory<\/a> on Maunakea and the <a href=\"http:\/\/pan-starrs.ifa.hawaii.edu\/public\/\">Pan-STARRS1 telescope<\/a> on Haleakala, as well as <a href=\"http:\/\/www.nasa.gov\/mission_pages\/swift\/main\/#.VG-EVihgu-8\">NASA&#8217;s Swift satellite<\/a>, has discovered an unusual source of light in a galaxy some 90 million light-years away. The team was led by <strong>Michael Koss<\/strong>, who was a postdoctoral fellow at the <a href=\"http:\/\/www.ifa.hawaii.edu\/\">Institute for Astronomy<\/a> at the <a href=\"http:\/\/manoa.hawaii.edu\/\">University of <span aria-label=\"Hawaii\">Hawai&#699;i<\/span> at M&#257;noa<\/a> during most of the time the study was ongoing.<\/p>\n<p>The object&#8217;s curious properties make it a good match for a supermassive black hole ejected from its home galaxy after merging with another giant black hole. But astronomers can&#8217;t yet rule out an alternative possibility. The source, called SDSS1133, may be the remnant of a massive star that underwent a record period of eruptions before destroying itself in a supernova explosion.<\/p>\n<p>&ldquo;With the data we have in hand, we can&#8217;t yet distinguish between these two scenarios,&rdquo; said Koss, now an astronomer at <a href=\"https:\/\/www.ethz.ch\/en.html\">ETH Zurich<\/a>, the Swiss Federal Institute of Technology. &ldquo;One exciting discovery made with NASA&#8217;s Swift is that the brightness of SDSS1133 hasn&#8217;t changed in ultraviolet light for a decade, which is not something typically seen in a young supernova remnant.&rdquo;<\/p>\n<p>In a study published in the November 21 edition of <em>Monthly Notices<\/em> of the Royal Astronomical Society, Koss and his colleagues report that the source has brightened significantly during the past six months, a trend that, if maintained, would bolster the black hole interpretation.<\/p>\n<p>To analyze the object in greater detail, the team is planning ultraviolet observations with the <a href=\"http:\/\/www.stsci.edu\/hst\/cos\">Cosmic Origins Spectrograph<\/a> aboard the Hubble Space Telescope in October 2015. &ldquo;We found in the Pan-STARRS1 imaging that SDSS1133 is getting significantly brighter over the last 6 months and that bolstered our case to study SDSS1133 now with HST,&rdquo; said <strong>Yanxia Li<\/strong> a <abbr>糖心视频<\/abbr> M&#257;noa graduate student involved in the analysis of the Pan-STARRS1 imaging in the study.<\/p>\n<p>Whatever SDSS1133 is, it&#8217;s persistent. The team was able to detect it in astronomical surveys dating back more than 60 years.<\/p>\n<p>&ldquo;We suspect we&#8217;re seeing the aftermath of a merger of two small galaxies and their central black holes,&rdquo; said co-author Laura Blecha, an Einstein Fellow in the <a href=\"http:\/\/www.astro.umd.edu\/\">University of Maryland&#8217;s Department of Astronomy<\/a> and a leading theorist in simulating recoils, or &ldquo;kicks,&rdquo; in merging black holes. &ldquo;Astronomers searching for recoiling black holes have been unable to confirm a detection, so finding even one of these sources would be a major discovery.&rdquo;<\/p>\n<p>&#8212;<em>For the full story, read the <a href=\"http:\/\/www.hawaii.edu\/news\/article.php?aId=6864\"><abbr>糖心视频<\/abbr> M&#257;noa news release<\/a><\/em>.<\/p>\n<p><em>&#8212;By Louise Good<\/em><\/p>\n","protected":false},"excerpt":{"rendered":"<p>Researchers study an unusual source of light in a galaxy some 90 million light-years 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