Astronomy and Astrophysics – Astrophysics
Scientific paper
2008-01-16
Astronomy and Astrophysics
Astrophysics
15 pages, ApJ in press
Scientific paper
10.1086/590899
The combination of a long duration and the absence of any accompanying supernova clearly shows that GRB 060614 can not be grouped into the two conventional classes of gamma-ray bursts, i.e. the long/soft bursts deemed to be collapsars and the short/hard bursts deemed to be merging binary compact stars. A new progenitor model is required for this anomalous gamma-ray burst. We propose that GRB 060614 might be produced through the tidal disruption of a star by an intermediate mass black hole. In this scenario, the long duration and the lack of any associated supernova are naturally expected. The theoretical energy output is also consistent with observations. The observed 9-s periodicity in the $\gamma$-ray light curve of GRB 060614 can also be satisfactorily explained.
Huang Yun-Feng
Lu Yi
Zhang Shuang Nan
No associations
LandOfFree
A tidal disruption model for the gamma-ray burst of GRB 060614 does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.
If you have personal experience with A tidal disruption model for the gamma-ray burst of GRB 060614, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and A tidal disruption model for the gamma-ray burst of GRB 060614 will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-159501