Multiwaveband analysis of brightest GRB070125
dc.contributor.author | Chandra, P. | |
dc.contributor.author | Cenko, S. | |
dc.contributor.author | Frail, D. | |
dc.contributor.author | Chevalier, R. | |
dc.contributor.author | Macquart, Jean-Pierre | |
dc.contributor.author | Kulkarni, S. | |
dc.contributor.author | Bock, D. | |
dc.contributor.author | Bertoldi, F. | |
dc.date.accessioned | 2017-01-30T11:09:47Z | |
dc.date.available | 2017-01-30T11:09:47Z | |
dc.date.created | 2016-09-12T08:36:36Z | |
dc.date.issued | 2008 | |
dc.identifier.citation | Chandra, P. and Cenko, S. and Frail, D. and Chevalier, R. and Macquart, J. and Kulkarni, S. and Bock, D. et al. 2008. Multiwaveband analysis of brightest GRB070125, pp. 346-349. | |
dc.identifier.uri | http://hdl.handle.net/20.500.11937/8966 | |
dc.identifier.doi | 10.1063/1.2943480 | |
dc.description.abstract |
We present a comprehensive multiwavelength analysis of the bright, long duration gamma-ray burst GRB 070125, comprised of observations in ?-ray, X-ray, optical, millimeter and centimeter wavebands. Radio light curves show rapid flux variations, which are interpreted as due to interstellar scintillation, and are used to derive an upper limit of 2.4×10 17cm on the radius of the fireball. Radio light curves and spectra suggest that the afterglow shock wave is moving in a dense medium. Our broadband modeling favors a constant density profile for the circumburst medium over a wind-like profile (R-2). GRB 070125 is a burst with high radiative efficiency (>60%). © 2008 American Institute of Physics. | |
dc.title | Multiwaveband analysis of brightest GRB070125 | |
dc.type | Conference Paper | |
dcterms.source.volume | 1000 | |
dcterms.source.startPage | 346 | |
dcterms.source.endPage | 349 | |
dcterms.source.title | AIP Conference Proceedings | |
dcterms.source.series | AIP Conference Proceedings | |
dcterms.source.isbn | 9780735405332 | |
curtin.department | Curtin Institute of Radio Astronomy (Physics) | |
curtin.accessStatus | Fulltext not available |
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