A mildly relativistic wide-angle outflow in the neutron-star merger event GW170817
GW170817 was the first gravitational-wave detection of a binary neutron-star merger1. It was accompanied by radiation across the electromagnetic spectrum and localized2 to the galaxy NGC 4993 at a distance of 40 megaparsecs. It has been proposed that the observed γ-ray, X-ray and radio emission is d...
| Main Authors: | Mooley, K., Nakar, E., Hotokezaka, K., Hallinan, G., Corsi, A., Frail, D., Horesh, A., Murphy, T., Lenc, E., Kaplan, D., De, K., Dobie, D., Chandra, P., Deller, A., Gottlieb, O., Kasliwal, M., Kulkarni, S., Myers, S., Nissanke, S., Piran, T., Lynch, Christene, Bhalerao, V., Bourke, S., Bannister, K., Singer, L. |
|---|---|
| Format: | Journal Article |
| Published: |
Nature Publishing Group
2018
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| Online Access: | http://hdl.handle.net/20.500.11937/70055 |
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