Journal article
A kilonova as the electromagnetic counterpart to a gravitational-wave source.
- Abstract:
-
Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can power an electromagnetic signal called a kilonova. The gravitational wave source GW170817 arose from a binary neutron star merger in the nearby Universe with a relatively well confined sky position and distance estimate6. Here we report observations and p...
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- Publication status:
- Published
- Peer review status:
- Peer reviewed
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Authors
Funding
Millennium Science Initiative
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Australian Research Council
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Bibliographic Details
- Publisher:
- Nature Publisher's website
- Journal:
- Nature Journal website
- Volume:
- 551
- Issue:
- 7678
- Pages:
- 75-79
- Publication date:
- 2017-10-16
- Acceptance date:
- 2017-09-25
- DOI:
- EISSN:
-
1476-4687
- ISSN:
-
0028-0836
- Pmid:
-
29094693
Item Description
- Language:
- English
- Keywords:
- Pubs id:
-
pubs:738048
- UUID:
-
uuid:60cc659f-3356-4289-ad34-f46b12bbb6b7
- Local pid:
- pubs:738048
- Source identifiers:
-
738048
- Deposit date:
- 2018-02-13
Terms of use
- Copyright holder:
- Macmillan Publishers Limited
- Copyright date:
- 2017
- Notes:
- © 2017 Macmillan Publishers Limited, part of Springer Nature. All rights reserved. This is the accepted manuscript version of the article. The final version is available online from Nature Publishing Group at: http://dx.doi.org/10.1038/nature24303
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