RADIO CONSTRAINTS ON LONG-LIVED MAGNETAR REMNANTS IN SHORT GAMMA-RAY BURSTS
The merger of a neutron star (NS) binary may result in the formation of a rapidly spinning magnetar. The magnetar can potentially survive for seconds or longer as a supramassive NS before collapsing to a black hole if, indeed, it collapses at all. During this process, a fraction of the magnetar'...
| Main Authors: | , , , |
|---|---|
| Other Authors: | |
| Language: | en |
| Published: |
IOP PUBLISHING LTD
2016
|
| Subjects: | |
| Online Access: | http://hdl.handle.net/10150/624065 http://arizona.openrepository.com/arizona/handle/10150/624065 |