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  SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin

Haberl, F., Sturm, R., Filipović, M. D., Pietsch, W., & Crawford, E. J. (2012). SXP 1062, a young Be X-ray binary pulsar with long spin period - implications for the neutron star birth spin. Astronomy & Astrophysics, 537: L1, pp. 1-5. doi:10.1051/0004-6361/201118369.

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Item Permalink: http://hdl.handle.net/11858/00-001M-0000-000F-8743-5 Version Permalink: http://hdl.handle.net/11858/00-001M-0000-0028-548D-4
Genre: Journal Article

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 Creators:
Haberl, F.1, Author              
Sturm, R.1, Author              
Filipović, M. D., Author
Pietsch, W.1, Author              
Crawford, E. J., Author
Affiliations:
1High Energy Astrophysics, MPI for Extraterrestrial Physics, Max Planck Society, ou_159890              

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Language(s): eng - English
 Dates: 2012-01
 Publication Status: Published in print
 Pages: -
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 Rev. Method: Peer
 Identifiers: DOI: 10.1051/0004-6361/201118369
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Title: Astronomy & Astrophysics
  Abbreviation : Astron. Astrophys.
Source Genre: Journal
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Pages: - Volume / Issue: 537 Sequence Number: L1 Start / End Page: 1 - 5 Identifier: ISSN: 0004-6361