- Abstract:
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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...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
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(pdf, 2.5MB)
-
- 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:
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pubs:666298
- URN:
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uri:8f0e6e70-46f1-4b76-bbe2-a9d90c8c3aca
- UUID:
-
uuid:8f0e6e70-46f1-4b76-bbe2-a9d90c8c3aca
- Local pid:
- pubs:666298
- Copyright holder:
- Podsiadlowski et al
- Copyright date:
- 2016
- Notes:
- © 2016 The Authors Published by Oxford University Press on behalf of the Royal Astronomical Society
Journal article
Light-curve and spectral properties of ultra-stripped core-collapse supernovae leading to binary neutron stars
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