A massive white-dwarf merger product before final collapse
A massive white-dwarf merger product before final collapse
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Publisher
London: Nature Publishing Group UK
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Language
English
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Publisher
London: Nature Publishing Group UK
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Contents
Gravitational-wave emission can lead to the coalescence of close pairs of compact objects orbiting each other
1
,
2
. In the case of neutron stars, such mergers may yield masses above the Tolman–Oppenheimer–Volkoff limit (2 to 2.7 solar masses)
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, leading to the formation of black holes
4
. For white dwarfs, the mass of the...
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Full title
A massive white-dwarf merger product before final collapse
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TN_cdi_proquest_miscellaneous_2232081595
Permalink
https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_miscellaneous_2232081595
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ISSN
0028-0836
E-ISSN
1476-4687
DOI
10.1038/s41586-019-1216-1