A new class of high-mass X-ray binaries: Implications for core collapse and 
neutron star recoil

Pfahl, E; Rappaport, S; Podsiadlowski, P; Spruit, H.

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A new class of high-mass X-ray binaries: Implications for core collapse and neutron star recoil

Pfahl, E., Rappaport, S., Podsiadlowski, P., & Spruit, H. (2002). A new class of high-mass X-ray binaries: Implications for core collapse and neutron star recoil. The Astrophysical Journal, 574(1), 364-376.

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Item Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-BB43-F Version Permalink: https://hdl.handle.net/11858/00-001M-0000-0011-BB44-D

Genre: Journal Article

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Creators:
Pfahl, E, Author
Rappaport, S, Author
Podsiadlowski, P, Author
Spruit, H.^{1, 2}, Author

Affiliations:
1Stellar Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159882
2High Energy Astrophysics, MPI for Astrophysics, Max Planck Society, ou_159881

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Free keywords: stars : neutron; supernovae : general; X-rays : stars

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Language(s): eng - English

Dates: Date issued: 2002

Publication Status: Issued

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Rev. Type: Peer

Identifiers: eDoc: 5509
ISI: 000176978200030

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Title: The Astrophysical Journal

Alternative Title : Astrophys. J.

Source Genre: Journal

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Pages: - Volume / Issue: 574 (1) Sequence Number: - Start / End Page: 364 - 376 Identifier: ISSN: 0004-637X