{"id":17096,"date":"2018-11-19T11:00:57","date_gmt":"2018-11-19T16:00:57","guid":{"rendered":"http:\/\/hobbyspace.com\/Blog\/?p=17096"},"modified":"2018-11-17T12:27:12","modified_gmt":"2018-11-17T17:27:12","slug":"eso-swirling-triple-star-system-may-generate-a-gamma-ray-burst","status":"publish","type":"post","link":"https:\/\/hobbyspace.com\/Blog\/?p=17096","title":{"rendered":"ESO: Swirling triple star system may generate a gamma-ray burst"},"content":{"rendered":"<p>A new report from <a title=\"Cosmic Serpent | ESO\" href=\"https:\/\/www.eso.org\/public\/news\/eso1838\/?lang\">ESO<\/a> (European Southern Observatory):<\/p>\n<p style=\"text-align: center;\"><strong><a title=\"Cosmic Serpent | ESO\" href=\"https:\/\/www.eso.org\/public\/news\/eso1838\/?lang\">Cosmic Serpent<\/a><\/strong><br \/>\n<em>ESO\u2019s VLT captures details of an elaborate serpentine system <\/em><br \/>\n<em>sculpted by colliding stellar winds<\/em><\/p>\n<p>The VISIR instrument on ESO\u2019s Very Large Telescope has captured this stunning image of a newly discovered massive triple star system. Nicknamed Apep after an ancient Egyptian deity, this may be the first ever gamma-ray burst progenitor found.<\/p>\n<p><figure id=\"attachment_17097\" aria-describedby=\"caption-attachment-17097\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/www.eso.org\/public\/images\/eso1838a\/\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" data-attachment-id=\"17097\" data-permalink=\"https:\/\/hobbyspace.com\/Blog\/?attachment_id=17097\" data-orig-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1.jpg\" data-orig-size=\"700,700\" data-comments-opened=\"0\" data-image-meta=\"{&quot;aperture&quot;:&quot;0&quot;,&quot;credit&quot;:&quot;ESO\/Callingham et al.&quot;,&quot;camera&quot;:&quot;&quot;,&quot;caption&quot;:&quot;The VISIR instrument on ESO\\u2019s VLT captured this stunning image of a newly-discovered massive binary star system. Nicknamed Apep after an ancient Egyptian deity, it could be the first gamma-ray burst progenitor to be found in our galaxy. Apep\\u2019s stellar winds have created the dust cloud surrounding the system, which consists of a binary star with a fainter companion. With 2 Wolf-Rayet stars orbiting each other in the binary, the serpentine swirls surrounding Apep are formed by the collision of two sets of powerful stellar winds, which create the spectacular dust plumes seen in the image. The reddish pinwheel in this image is data from the VISIR instrument on ESO\\u2019s Very Large Telescope (VLT), and shows the spectacular plumes of dust surrounding Apep. The blue sources at the centre of the image are a triple star system \\u2014 which consists of a binary star system and a companion single star bound together by gravity. Though only two star-like objects are visible in the image, the lower source is in fact an unresolved binary Wolf-Rayet star. The triple star system was captured by the NACO adaptive optics instrument on the VLT.&quot;,&quot;created_timestamp&quot;:&quot;1542646800&quot;,&quot;copyright&quot;:&quot;&quot;,&quot;focal_length&quot;:&quot;0&quot;,&quot;iso&quot;:&quot;0&quot;,&quot;shutter_speed&quot;:&quot;0&quot;,&quot;title&quot;:&quot;Coils of Apep&quot;,&quot;orientation&quot;:&quot;0&quot;}\" data-image-title=\"Coils of Apep\" data-image-description=\"\" data-image-caption=\"&lt;p&gt;The VISIR instrument on ESO\u2019s VLT captured this stunning image of a newly-discovered massive binary star system. Nicknamed Apep after an ancient Egyptian deity, it could be the first gamma-ray burst progenitor to be found in our galaxy. Apep\u2019s stellar winds have created the dust cloud surrounding the system, which consists of a binary star with a fainter companion. With 2 Wolf-Rayet stars orbiting each other in the binary, the serpentine swirls surrounding Apep are formed by the collision of two sets of powerful stellar winds, which create the spectacular dust plumes seen in the image. The reddish pinwheel in this image is data from the VISIR instrument on ESO\u2019s Very Large Telescope (VLT), and shows the spectacular plumes of dust surrounding Apep. The blue sources at the centre of the image are a triple star system \u2014 which consists of a binary star system and a companion single star bound together by gravity. Though only two star-like objects are visible in the image, the lower source is in fact an unresolved binary Wolf-Rayet star. The triple star system was captured by the NACO adaptive optics instrument on the VLT.&lt;\/p&gt;\n\" data-large-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1.jpg\" class=\"wp-image-17097\" src=\"http:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1.jpg\" alt=\"\" width=\"500\" height=\"500\" srcset=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1.jpg 700w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1-150x150.jpg 150w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838a1-300x300.jpg 300w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-17097\" class=\"wp-caption-text\"><em>The VISIR instrument on ESO\u2019s VLT captured this stunning image of a newly-discovered massive binary star system. Nicknamed Apep after an ancient Egyptian deity, it could be the first gamma-ray burst progenitor to be found in our galaxy. Apep\u2019s stellar winds have created the dust cloud surrounding the system, which consists of a binary star with a fainter companion. With 2 Wolf-Rayet stars orbiting each other in the binary, the serpentine swirls surrounding Apep are formed by the collision of two sets of powerful stellar winds, which create the spectacular dust plumes seen in the image. The reddish pinwheel in this image is data from the VISIR instrument on ESO\u2019s Very Large Telescope (VLT), and shows the spectacular plumes of dust surrounding Apep. The blue sources at the centre of the image are a triple star system \u2014 which consists of a binary star system and a companion single star bound together by gravity. Though only two star-like objects are visible in the image, the lower source is in fact an unresolved binary Wolf-Rayet star. The triple star system was captured by the NACO adaptive optics instrument on the VLT. [<a href=\"https:\/\/www.eso.org\/public\/images\/eso1838a\/\">Higher-res image files<\/a>]<br \/><\/em><\/figcaption><\/figure>This serpentine swirl, captured by the <a href=\"https:\/\/www.eso.org\/public\/teles-instr\/paranal-observatory\/vlt\/vlt-instr\/visir\/\">VISIR<\/a> instrument on ESO\u2019s <a href=\"https:\/\/www.eso.org\/public\/teles-instr\/paranal-observatory\/vlt\/\">Very Large Telescope<\/a> (VLT), has an explosive future ahead of it; it is a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Wolf%E2%80%93Rayet_star\">Wolf-Rayet star<\/a> system, and a likely source of one of the most energetic phenomena in the Universe \u2014 a long-duration <a href=\"https:\/\/www.eso.org\/public\/science\/grb\/\">gamma-ray burst<\/a> (GRB).<\/p>\n<p style=\"padding-left: 30px;\">\u201c<em>This is the first such system to be discovered in our own galaxy<\/em>,\u201d explains Joseph Callingham of the Netherlands Institute for Radio Astronomy (<a href=\"https:\/\/www.astron.nl\/\">ASTRON<\/a>), lead author of the study reporting this system. \u201c<em>We never expected to find such a system in our own backyard<\/em>\u201d <a href=\"#1\">[1]<\/a>.<\/p>\n<p dir=\"ltr\">The system, which comprises a nest of massive stars surrounded by a \u201cpinwheel\u201d of dust, is \u00a0officially known only by unwieldy catalogue references like 2XMM J160050.7-514245. However, the astronomers chose to give this fascinating object a catchier moniker \u2014 \u201cApep\u201d.<\/p>\n<p><span class=\"embed-youtube\" style=\"text-align:center; display: block;\"><iframe loading=\"lazy\" class=\"youtube-player\" width=\"1600\" height=\"900\" src=\"https:\/\/www.youtube.com\/embed\/CqTWI-qCP44?version=3&#038;rel=1&#038;showsearch=0&#038;showinfo=1&#038;iv_load_policy=1&#038;fs=1&#038;hl=en&#038;autohide=2&#038;wmode=transparent\" allowfullscreen=\"true\" style=\"border:0;\" sandbox=\"allow-scripts allow-same-origin allow-popups allow-presentation allow-popups-to-escape-sandbox\"><\/iframe><\/span><\/p>\n<p>Apep got its nickname for its sinuous shape, reminiscent of a snake coiled around the central stars. Its namesake was an <a href=\"https:\/\/en.wikipedia.org\/wiki\/Apep\">ancient Egyptian deity<\/a>, a gargantuan serpent embodying chaos \u2014 fitting for such a violent system. It was believed that Ra, the Sun god, would battle with Apep every night; prayer and worship ensured Ra\u2019s victory and the return of the Sun.<\/p>\n<p>GRBs are among the most powerful explosions in the Universe. Lasting between a few thousandths of a second and a few hours, they can release as much energy as the Sun will output over its entire lifetime. Long-duration GRBs \u2014 those which last for longer than 2 seconds \u2014 are believed to be caused by the supernova explosions of rapidly-rotating Wolf-Rayet stars.<\/p>\n<p>Some of the most massive stars <a href=\"https:\/\/en.wikipedia.org\/wiki\/Stellar_evolution\">evolve<\/a> into Wolf-Rayet stars towards the end of their lives. This stage is short-lived, and Wolf-Rayets survive in this state for only a few hundred thousand years \u2014 the blink of an eye in cosmological terms. In that time, they throw out huge amounts of material in the form of a powerful <a href=\"https:\/\/en.wikipedia.org\/wiki\/Stellar_wind\">stellar wind<\/a>, hurling matter outwards at millions of kilometres per hour; Apep\u2019s stellar winds were measured to travel at an astonishing 12 million km\/h.<\/p>\n<p>These stellar winds have created the elaborate plumes surrounding the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Star_system#Triple_star_systems\">triple star system<\/a> \u2014 which consists of a <a href=\"https:\/\/en.wikipedia.org\/wiki\/Binary_star\">binary<\/a> star system and a companion single star bound together by gravity. Though only two star-like objects are visible in the image, the lower source is in fact an unresolved binary Wolf-Rayet star. This binary is responsible for sculpting the serpentine swirls surrounding Apep, which are formed in the wake of the colliding stellar winds from the two Wolf-Rayet stars.<\/p>\n<p>Compared to the extraordinary speed of Apep\u2019s winds, the dust pinwheel itself swirls outwards at a leisurely pace, \u201ccrawling\u201d along at less than 2 million km\/h. The wild discrepancy between the speed of Apep\u2019s rapid stellar winds and that of the unhurried dust pinwheel is thought to result from one of the stars in the binary launching both a fast and a slow wind \u2014 in different directions.<\/p>\n<p>This would imply that the star is undergoing near-critical rotation \u2014 that is, rotating so fast that it is nearly ripping itself apart. A Wolf-Rayet star with such rapid rotation is believed to produce a long-duration GRB when its core collapses at the end of its life.<\/p>\n<p><figure id=\"attachment_17098\" aria-describedby=\"caption-attachment-17098\" style=\"width: 500px\" class=\"wp-caption aligncenter\"><a href=\"https:\/\/www.eso.org\/public\/images\/eso1838c\/\" target=\"_blank\" rel=\"noopener\"><img loading=\"lazy\" decoding=\"async\" data-attachment-id=\"17098\" data-permalink=\"https:\/\/hobbyspace.com\/Blog\/?attachment_id=17098\" data-orig-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838c1.jpg\" data-orig-size=\"700,543\" data-comments-opened=\"0\" data-image-meta=\"{&quot;aperture&quot;:&quot;0&quot;,&quot;credit&quot;:&quot;ESO\/Digitized Sky Survey 2. Ackn&quot;,&quot;camera&quot;:&quot;&quot;,&quot;caption&quot;:&quot;The image is a colour composite made from exposures from the Digitized Sky Survey 2 (DSS2), and shows the region surrounding\\u00a0 2XMM J160050.7-514245, nicknamed \\u201cApep\\u201d. The field of view is approximately 2.4 x 2.0 degrees. \\u00a0&quot;,&quot;created_timestamp&quot;:&quot;1542646800&quot;,&quot;copyright&quot;:&quot;&quot;,&quot;focal_length&quot;:&quot;0&quot;,&quot;iso&quot;:&quot;0&quot;,&quot;shutter_speed&quot;:&quot;0&quot;,&quot;title&quot;:&quot;Digitized Sky Survey image around Apep&quot;,&quot;orientation&quot;:&quot;0&quot;}\" data-image-title=\"Digitized Sky Survey image around Apep\" data-image-description=\"\" data-image-caption=\"&lt;p&gt;The image is a colour composite made from exposures from the Digitized Sky Survey 2 (DSS2), and shows the region surrounding\u00a0 2XMM J160050.7-514245, nicknamed \u201cApep\u201d. The field of view is approximately 2.4 x 2.0 degrees. \u00a0&lt;\/p&gt;\n\" data-large-file=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838c1.jpg\" class=\"wp-image-17098\" src=\"http:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838c1.jpg\" alt=\"\" width=\"500\" height=\"388\" srcset=\"https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838c1.jpg 700w, https:\/\/hobbyspace.com\/Blog\/wp-content\/uploads\/2018\/11\/eso1838c1-300x233.jpg 300w\" sizes=\"auto, (max-width: 500px) 100vw, 500px\" \/><\/a><figcaption id=\"caption-attachment-17098\" class=\"wp-caption-text\"><em>The image is a colour composite made from exposures from the Digitized Sky Survey 2 (DSS2), and shows the region surrounding\u00a0 2XMM J160050.7-514245, nicknamed \u201cApep\u201d. The field of view is approximately 2.4 x 2.0 degrees. [<a href=\"https:\/\/www.eso.org\/public\/images\/eso1838c\/\">Higher-res image files<\/a>]<br \/><\/em><\/figcaption><\/figure><strong>Notes<\/strong><br \/>\n<a class=\"anchor\" name=\"1\"><\/a>[1] Callingham, now at the Netherlands Institute for Radio Astronomy (<a href=\"https:\/\/www.astron.nl\/\">ASTRON<\/a>), did part of this research while at the University of Sydney working with research team leader Peter Tuthill. In addition to observations from ESO telescopes, the team also used the <a href=\"https:\/\/en.wikipedia.org\/wiki\/Anglo-Australian_Telescope\">Anglo-Australian Telescope<\/a> at <a href=\"https:\/\/en.wikipedia.org\/wiki\/Siding_Spring_Observatory\">Siding Spring Observatory<\/a>, Australia.<\/p>\n<p><strong>Links<\/strong><\/p>\n<ul>\n<li><a href=\"https:\/\/www.eso.org\/public\/archives\/releases\/sciencepapers\/eso1838\/eso1838a.pdf\">Research paper<\/a><\/li>\n<li><a href=\"http:\/\/www.eso.org\/public\/images\/archive\/category\/paranal\/\">Photos of the VLT<\/a><\/li>\n<li><a href=\"https:\/\/astronomycommunity.nature.com\/users\/181582-joseph-callingham\/posts\/40890-riding-the-serpent-the-discovery-and-study-of-apep\">Behind the Paper blog post<\/a><\/li>\n<\/ul>\n","protected":false},"excerpt":{"rendered":"<p>A new report from ESO (European Southern Observatory): Cosmic Serpent ESO\u2019s VLT captures details of an elaborate serpentine system sculpted by colliding stellar winds The VISIR instrument on ESO\u2019s Very Large Telescope has captured this stunning image of a newly discovered massive triple star system. Nicknamed Apep after an ancient Egyptian deity, this may be &hellip; <a href=\"https:\/\/hobbyspace.com\/Blog\/?p=17096\" class=\"more-link\">Continue reading <span class=\"screen-reader-text\">ESO: Swirling triple star system may generate a gamma-ray burst<\/span> <span class=\"meta-nav\">&rarr;<\/span><\/a><\/p>\n","protected":false},"author":1,"featured_media":0,"comment_status":"closed","ping_status":"open","sticky":false,"template":"","format":"standard","meta":{"_jetpack_newsletter_access":"","_jetpack_dont_email_post_to_subs":false,"_jetpack_newsletter_tier_id":0,"_jetpack_memberships_contains_paywalled_content":false,"_jetpack_memberships_contains_paid_content":false,"footnotes":"","jetpack_post_was_ever_published":false},"categories":[12],"tags":[],"class_list":["post-17096","post","type-post","status-publish","format-standard","hentry","category-astronomy"],"jetpack_featured_media_url":"","jetpack_sharing_enabled":true,"jetpack_shortlink":"https:\/\/wp.me\/p34aWK-4rK","jetpack-related-posts":[{"id":20544,"url":"https:\/\/hobbyspace.com\/Blog\/?p=20544","url_meta":{"origin":17096,"position":0},"title":"ESO: VLT detects ancient burst of star formation in Milky Way core","author":"TopSpacer","date":"December 16, 2019","format":false,"excerpt":"A new report from the European Southern Observatory (ESO): ESO Telescope Images Stunning Central Region of Milky Way, Finds Ancient Star Burst ESO\u2019s Very Large Telescope (VLT) has observed the central part of the Milky Way with spectacular resolution and uncovered new details about the history of star birth in\u2026","rel":"","context":"In &quot;Astronomy&quot;","block_context":{"text":"Astronomy","link":"https:\/\/hobbyspace.com\/Blog\/?cat=12"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2019\/12\/eso1920a1-500x216.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":13727,"url":"https:\/\/hobbyspace.com\/Blog\/?p=13727","url_meta":{"origin":17096,"position":1},"title":"ESO: Very Large Telescope to search for planets in Alpha Centauri system","author":"TopSpacer","date":"January 9, 2017","format":false,"excerpt":"Here is a new article from\u00a0ESO\u00a0(European Southern Observatory): VLT to Search for Planets in Alpha Centauri System ESO has signed an agreement with the Breakthrough Initiatives to adapt the Very Large Telescope instrumentation in Chile to conduct a search for planets in the nearby star system Alpha Centauri. Such planets\u2026","rel":"","context":"In &quot;Astronomy&quot;","block_context":{"text":"Astronomy","link":"https:\/\/hobbyspace.com\/Blog\/?cat=12"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2017\/01\/eso1702a1.jpg?resize=350%2C200","width":350,"height":200},"classes":[]},{"id":24731,"url":"https:\/\/hobbyspace.com\/Blog\/?p=24731","url_meta":{"origin":17096,"position":2},"title":"ESO: VLT spots planet orbiting most massive star pair so far","author":"TopSpacer","date":"December 8, 2021","format":false,"excerpt":"The latest report from the European Southern Observatory (ESO): ESO telescope images planet around most massive star pair to date The European Southern Observatory\u2019s Very Large Telescope (ESO\u2019s VLT) has captured an image of a planet orbiting b Centauri, a two-star system that can be seen with the naked eye.\u2026","rel":"","context":"In &quot;Astronomy&quot;","block_context":{"text":"Astronomy","link":"https:\/\/hobbyspace.com\/Blog\/?cat=12"},"img":{"alt_text":"","src":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/12\/eso2118c1.jpg?resize=350%2C200&ssl=1","width":350,"height":200,"srcset":"https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/12\/eso2118c1.jpg?resize=350%2C200&ssl=1 1x, https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/12\/eso2118c1.jpg?resize=525%2C300&ssl=1 1.5x, https:\/\/i0.wp.com\/hobbyspace.com\/Blog\/wp-content\/uploads\/2021\/12\/eso2118c1.jpg?resize=700%2C400&ssl=1 2x"},"classes":[]},{"id":16901,"url":"https:\/\/hobbyspace.com\/Blog\/?p=16901","url_meta":{"origin":17096,"position":3},"title":"ESO: Watching stars form in the Skull and Crossbones Nebula","author":"TopSpacer","date":"October 24, 2018","format":false,"excerpt":"The latest report from the European Southern Observatrory (ESO): The Pirate of the Southern Skies FORS2, an instrument mounted on ESO\u2019s Very Large Telescope, has observed the active star-forming region NGC 2467 \u2014 sometimes referred to as the Skull and Crossbones Nebula. 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