Journal article
Luminous Blue Variables and superluminous supernovae from binary mergers
- Abstract:
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Evidence suggests that the direct progenitor stars of some core-collapse supernovae (CCSNe) are luminous blue variables (LBVs), perhaps including some `superluminous supernovae' (SLSNe). We examine models in which massive stars gain mass soon after the end of core hydrogen burning. These are mainly intended to represent mergers following a brief contact phase during early Case B mass transfer, but may also represent stars which gain mass in the Hertzsprung Gap or extremely late during the mai...
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- Publication status:
- Published
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- Publisher copy:
- 10.1088/0004-637X/796/2/121
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Authors
Bibliographic Details
- Journal:
- ASTROPHYSICAL JOURNAL
- Volume:
- 796
- Issue:
- 2
- Publication date:
- 2014-10-09
- DOI:
- ISSN:
-
0004-637X
- Source identifiers:
-
486112
Item Description
- Keywords:
- Pubs id:
-
pubs:486112
- UUID:
-
uuid:0ad1df67-5f55-40e4-9fd8-e771958f26c1
- Local pid:
- pubs:486112
- Deposit date:
- 2014-10-10
Terms of use
- Copyright date:
- 2014
- Notes:
- Accepted to The Astrophysical Journal. 24 pages
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