Journal article

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

Publication status:: Published

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APA Style

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. ASTROPHYSICAL JOURNAL, 574(1), 364–376.

MLA Style

Pfahl, E, et al. “A New Class of High-Mass X-Ray Binaries: Implications for Core Collapse and Neutron Star Recoil.” ASTROPHYSICAL JOURNAL, vol. 574, no. 1, 2002, pp. 364–76.

Chicago Style

Pfahl, E, S Rappaport, P Podsiadlowski, and H Spruit. 2002. “A New Class of High-Mass X-Ray Binaries: Implications for Core Collapse and Neutron Star Recoil.” ASTROPHYSICAL JOURNAL 574 (1): 364–76.
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Publisher copy:: 10.1086/340794

Authors

+ Pfahl, E More by this author

Role:: Author

+ Rappaport, S More by this author

Role:: Author

+ Podsiadlowski, P More by this author

Institution:: University of Oxford
Division:: MPLS
Department:: Physics
Sub department:: Astrophysics
Role:: Author

+ Spruit, H More by this author

Role:: Author

Journal:: ASTROPHYSICAL JOURNAL More from this journal
Volume:: 574
Issue:: 1
Pages:: 364-376
Publication date:: 2002-07-20
DOI:: 10.1086/340794
EISSN:: 1538-4357
ISSN:: 0004-637X

Keywords:: stars : neutron

supernovae : general

X-rays : stars
Pubs id:: pubs:18571
UUID:: uuid:51f33c07-6b6b-4fac-9a0d-43e4b585f9f8
Local pid:: pubs:18571
Source identifiers:: 18571
Deposit date:: 2012-12-19
ARK identifier:: ark:/29072/ora_51f33c076b6b4fac9a0d43e4b585f9f8

Terms of use

Copyright date:: 2002

Licence:: Terms and Conditions of Use for Oxford University Research Archive

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