GRB 130603B: No Compelling Evidence for Neutron Star Merger
Abstract
Near infrared (NIR) flare/rebrightening in the afterglow of the short hard gamma ray burst (SHB) 130603B measured with the Hubble Space Telescope (HST) and an alleged late-time X-ray excess were interpreted as possible evidence of a neutron-star merger origin of this SHB. However, the X-ray afterglow that was measured with the Swift-XRT and Newton XMM have the canonical behaviour of a synchrotron afterglow produced by a highly relativistic jet. The H-band flux observed with HST 9.41 days after burst is that expected from the measured late-time X-ray afterglow. A late-time flare/re-brightening of a NIR-Optical afterglow of SHB can be produced by jet collision with an interstellar density bump, or by a kilonova, but jet plus kilonova can be produced also by the collapse of compact stars (neutron star, strange star, or quark star) to a more compact object due to cooling, loss of angular momentum, or mass accretion.
- Publication:
-
Advances in Astronomy
- Pub Date:
- 2015
- DOI:
- 10.1155/2015/460293
- arXiv:
- arXiv:1402.5542
- Bibcode:
- 2015AdAst2015E..16D
- Keywords:
-
- Astrophysics - High Energy Astrophysical Phenomena
- E-Print:
- 8 pages, 1 figure