Pulsational pair instability as an explanation for the most luminous supernovae

Woosley, S. E.; Blinnikov, S.; Heger, A.

doi:10.1038/nature06333

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Pulsational pair instability as an explanation for the most luminous supernovae

Woosley, S. E., Blinnikov, S., & Heger, A. (2007). Pulsational pair instability as an explanation for the most luminous supernovae. Nature, 450(7168), 390-392. doi:10.1038/nature06333.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-A8F1-D Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-A8F2-B

Genre: Journal Article

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Woosley, S. E., Author
Blinnikov, S.¹, Author
Heger, A., Author

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1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882

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Language(s): eng - English

Dates: Date issued: 2007-11-15

Publication Status: Issued

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Identifiers: eDoc: 324286
DOI: 10.1038/nature06333

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Title: Nature

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Pages: - Volume / Issue: 450 (7168) Sequence Number: - Start / End Page: 390 - 392 Identifier: ISSN: 0028-0836