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Conference Paper: The late-time detections of the X-ray afterglow of GRB 060729 with Chandra

TitleThe late-time detections of the X-ray afterglow of GRB 060729 with Chandra
Authors
KeywordsGamma-ray bursts
Issue Date2011
Citation
Aip Conference Proceedings, 2011, v. 1358, p. 125-129 How to Cite?
AbstractWe summarize the results of the late-time Chandra observations of the X-ray afterglow of the Swift-discovered GRB 060729. These Chandra observations have been the latest X-ray detections of an afterglow even, up to 21 month after the trigger. The last two Chandra observations in December 2007 and May 2008 suggest a break at about a year after the burst, implying a jet half-opening angle of about 14 degrees, if interpreted as a jet break. As an alternative this break may have a spectral origin. In that case no jet break was observed and the half-opening angle is larger than 15 degrees for a wind medium. Comparing the X-ray afterglow of GRB 060729 with other bright X-ray afterglows we discuss why the afterglow of GRB 060729 was such an exceptionally long-lasting event. The detection by Chandra in May 2008 was the latest detection of an X-ray afterglow at cosmological distance ever. © 2011 American Institute of Physics.
Persistent Identifierhttp://hdl.handle.net/10722/361187
ISSN
2023 SCImago Journal Rankings: 0.152

 

DC FieldValueLanguage
dc.contributor.authorGrupe, Dirk-
dc.contributor.authorBurrows, Dave-
dc.contributor.authorWu, Xue Feng-
dc.contributor.authorZhang, Bing-
dc.contributor.authorGarmire, Gordon-
dc.date.accessioned2025-09-16T04:15:12Z-
dc.date.available2025-09-16T04:15:12Z-
dc.date.issued2011-
dc.identifier.citationAip Conference Proceedings, 2011, v. 1358, p. 125-129-
dc.identifier.issn0094-243X-
dc.identifier.urihttp://hdl.handle.net/10722/361187-
dc.description.abstractWe summarize the results of the late-time Chandra observations of the X-ray afterglow of the Swift-discovered GRB 060729. These Chandra observations have been the latest X-ray detections of an afterglow even, up to 21 month after the trigger. The last two Chandra observations in December 2007 and May 2008 suggest a break at about a year after the burst, implying a jet half-opening angle of about 14 degrees, if interpreted as a jet break. As an alternative this break may have a spectral origin. In that case no jet break was observed and the half-opening angle is larger than 15 degrees for a wind medium. Comparing the X-ray afterglow of GRB 060729 with other bright X-ray afterglows we discuss why the afterglow of GRB 060729 was such an exceptionally long-lasting event. The detection by Chandra in May 2008 was the latest detection of an X-ray afterglow at cosmological distance ever. © 2011 American Institute of Physics.-
dc.languageeng-
dc.relation.ispartofAip Conference Proceedings-
dc.subjectGamma-ray bursts-
dc.titleThe late-time detections of the X-ray afterglow of GRB 060729 with Chandra-
dc.typeConference_Paper-
dc.description.naturelink_to_subscribed_fulltext-
dc.identifier.doi10.1063/1.3621753-
dc.identifier.scopuseid_2-s2.0-80052490735-
dc.identifier.volume1358-
dc.identifier.spage125-
dc.identifier.epage129-
dc.identifier.eissn1551-7616-

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