Ultra-stripped supernovae: progenitors and fate
The explosion of ultra-stripped stars in close binaries can lead to ejecta masses <0.1 M⊙ and may explain some of the recent discoveries of weak and fast optical transients. In Tauris et al., it was demonstrated that helium star companions to neutron stars (NSs) may experience mass transfer a...
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| Format: | Journal article |
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Oxford University Press
2015
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