Astronomy and Astrophysics – Astrophysics
Scientific paper
2006-08-11
Nature 444:1053-1055,2006
Astronomy and Astrophysics
Astrophysics
Scientific paper
10.1038/nature05373
Over the past decade our physical understanding of gamma-ray bursts (GRBs) has progressed rapidly thanks to the discovery and observation of their long-lived afterglow emission. Long-duration (T < 2 s) GRBs are associated with the explosive deaths of massive stars (``collapsars''), which produce accompanying supernovae, while the short-duration (T > 2 s) GRBs arise from a different origin, which has been argued to be the merger of two compact objects, either neutron stars or black holes. Here we present observations of GRB060614, a 100-s long burst discovered by the Swift satellite, which require the invocation of a new explosive process: either a massive ``collapsar'' that powers a GRB without any associated supernova, or a new type of engine, as long-lived as the collapsar but without any such massive stellar host. We also discuss the properties of this burst's redshift z=0.125 host galaxy, which distinguish it from other long-duration GRBs and suggest that an entirely new type of GRB progenitor may be required.
Berger Edmond
Brown Patrick
Burrows David
Cenko Brad
Chevalier Roger
No associations
LandOfFree
The gamma-ray burst GRB060614 requires a novel explosive process 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 The gamma-ray burst GRB060614 requires a novel explosive process, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The gamma-ray burst GRB060614 requires a novel explosive process will most certainly appreciate the feedback.
Profile ID: LFWR-SCP-O-586547