Show simple item record

Swift and optical observations of GRB 050401

dc.contributor.authorMason, KO
dc.contributor.authorBeardmore, AP
dc.contributor.authorBarthelmy, SD
dc.contributor.authorBoyd, P
dc.contributor.authorBurrows, DN
dc.contributor.authorFink, R
dc.contributor.authorGehrels, N
dc.contributor.authorKobayashi, S
dc.contributor.authorMcNought, R
dc.contributor.authorNousek, JA
dc.contributor.authorPage, KL
dc.contributor.authorPalmer, DM
dc.contributor.authorPeterson, BA
dc.contributor.authorPrice, PA
dc.contributor.authorRich, J
dc.contributor.authorRoming, P
dc.contributor.authorRosen, SR
dc.contributor.authorSakamoto, T
dc.contributor.authorSchmidt, BP
dc.contributor.authorTueller, J
dc.contributor.authorWells, AA
dc.contributor.authorZane, S
dc.contributor.authorZhang, B
dc.contributor.authorZiaeepour, H
dc.contributor.authorDe Pasquale, M
dc.date.accessioned2021-03-04T10:48:25Z
dc.date.available2021-03-04T10:48:25Z
dc.date.issued2006
dc.identifier.citationDe Pasquale M., Beardmore A., Barthelmy S., Boyd P., Burrows D., Fink R., Gehrels N., Kobayashi S., Mason K., McNought R., et al., "Swift and optical observations of GRB 050401", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.365, sa.3, ss.1031-1038, 2006
dc.identifier.issn0035-8711
dc.identifier.othervv_1032021
dc.identifier.otherav_6f14fc52-d761-4cc7-8454-bd001a093929
dc.identifier.urihttp://hdl.handle.net/20.500.12627/76677
dc.identifier.urihttps://doi.org/10.1111/j.1365-2966.2005.09787.x
dc.description.abstractWe present the results of the analysis of gamma-ray and X-ray data of GRB 050401 taken with the Swift satellite, together with a series of ground-based follow-up optical observations. The Swift X-ray light curve shows a clear break at about 4900 s after the gamma-ray burst (GRB). The decay indices before and after the break are consistent with a scenario of continuous injection of radiation from the 'central engine' of the GRB to the fireball. Alternatively, this behaviour could result if ejecta are released with a range of Lorentz factors, with the slower shells catching up the faster at the afterglow shock position. The two scenarios are observationally indistinguishable.
dc.language.isoeng
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.titleSwift and optical observations of GRB 050401
dc.typeMakale
dc.relation.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.contributor.department, ,
dc.identifier.volume365
dc.identifier.issue3
dc.identifier.startpage1031
dc.identifier.endpage1038
dc.contributor.firstauthorID103362


Files in this item

FilesSizeFormatView

There are no files associated with this item.

This item appears in the following Collection(s)

Show simple item record