Reverse Shock Emission from Short GRBs
We investigate the expected radio emission from the reverse shock of short GRBs, using the fitted afterglow parameters. In light of recent results suggesting that in some cases the radio afterglow is due to emission from the reverse shock, we examine the extent to which this component is detectable...
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| Format: | Article |
| Language: | English |
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MDPI AG
2018-09-01
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| Series: | Galaxies |
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| Online Access: | http://www.mdpi.com/2075-4434/6/4/103 |