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Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars

Abstract:

We investigate light-curve and spectral properties of ultra-stripped core-collapse supernovae. Ultra-stripped supernovae are the explosions of heavily stripped massive stars which lost their envelopes via binary interactions with a compact companion star. They eject only ∼0.1~M⊙ and may be the main way to form double neutron-star systems which eventually merge emitting strong gravitational waves. We follow the evolution of an ultra-stripped supernova progenitor until iron core collapse and pe...

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Publication status:
Published
Peer review status:
Peer reviewed
Version:
Publisher's version

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Publisher copy:
10.1093/mnras/stw3225

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Publisher:
Oxford University Press Publisher's website
Journal:
Monthly Notices of the Royal Astronomical Society Journal website
Volume:
466
Issue:
2
Pages:
2085–2098
Publication date:
2016-12-05
Acceptance date:
2016-12-08
DOI:
Pubs id:
pubs:666298
URN:
uri:8f0e6e70-46f1-4b76-bbe2-a9d90c8c3aca
UUID:
uuid:8f0e6e70-46f1-4b76-bbe2-a9d90c8c3aca
Local pid:
pubs:666298

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