Journal article
Hydrogen-poor superluminous stellar explosions.
- Abstract:
-
Supernovae are stellar explosions driven by gravitational or thermonuclear energy that is observed as electromagnetic radiation emitted over weeks or more. In all known supernovae, this radiation comes from internal energy deposited in the outflowing ejecta by one or more of the following processes: radioactive decay of freshly synthesized elements (typically (56)Ni), the explosion shock in the envelope of a supergiant star, and interaction between the debris and slowly moving, hydrogen-rich ...
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- Publication status:
- Published
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- Publisher copy:
- 10.1038/nature10095
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Authors
Bibliographic Details
- Journal:
- Nature
- Volume:
- 474
- Issue:
- 7352
- Pages:
- 487-489
- Publication date:
- 2011-06-01
- DOI:
- EISSN:
-
1476-4687
- ISSN:
-
0028-0836
- Source identifiers:
-
164266
Item Description
- Language:
- English
- Pubs id:
-
pubs:164266
- UUID:
-
uuid:36346c3d-2409-42e2-9499-444e805fe6e6
- Local pid:
- pubs:164266
- Deposit date:
- 2012-12-19
Terms of use
- Copyright date:
- 2011
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