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Conference Paper: The late-time detections of the X-ray afterglow of GRB 060729 with Chandra
| Title | The late-time detections of the X-ray afterglow of GRB 060729 with Chandra |
|---|---|
| Authors | |
| Keywords | Gamma-ray bursts |
| Issue Date | 2011 |
| Citation | Aip Conference Proceedings, 2011, v. 1358, p. 125-129 How to Cite? |
| Abstract | We 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 Identifier | http://hdl.handle.net/10722/361187 |
| ISSN | 2023 SCImago Journal Rankings: 0.152 |
| DC Field | Value | Language |
|---|---|---|
| dc.contributor.author | Grupe, Dirk | - |
| dc.contributor.author | Burrows, Dave | - |
| dc.contributor.author | Wu, Xue Feng | - |
| dc.contributor.author | Zhang, Bing | - |
| dc.contributor.author | Garmire, Gordon | - |
| dc.date.accessioned | 2025-09-16T04:15:12Z | - |
| dc.date.available | 2025-09-16T04:15:12Z | - |
| dc.date.issued | 2011 | - |
| dc.identifier.citation | Aip Conference Proceedings, 2011, v. 1358, p. 125-129 | - |
| dc.identifier.issn | 0094-243X | - |
| dc.identifier.uri | http://hdl.handle.net/10722/361187 | - |
| dc.description.abstract | We 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.language | eng | - |
| dc.relation.ispartof | Aip Conference Proceedings | - |
| dc.subject | Gamma-ray bursts | - |
| dc.title | The late-time detections of the X-ray afterglow of GRB 060729 with Chandra | - |
| dc.type | Conference_Paper | - |
| dc.description.nature | link_to_subscribed_fulltext | - |
| dc.identifier.doi | 10.1063/1.3621753 | - |
| dc.identifier.scopus | eid_2-s2.0-80052490735 | - |
| dc.identifier.volume | 1358 | - |
| dc.identifier.spage | 125 | - |
| dc.identifier.epage | 129 | - |
| dc.identifier.eissn | 1551-7616 | - |
