THE Be/X-RAY BINARY SWIFT J1626.6-5156 AS A VARIABLE CYCLOTRON LINE SOURCE

Record Type
Journal Articles
Full Title
THE Be/X-RAY BINARY SWIFT J1626.6-5156 AS A VARIABLE CYCLOTRON LINE SOURCE
Author(s)
DeCesar M, Boyd P, Pottschmidt K, Wilms J, Suchy S, Miller M
Publication Title
ASTROPHYSICAL JOURNAL
Publication Title (abbreviated)
ASTROPHYS J
Publication Date
2013 Jan 1
DOI
10.1088/0004-637X/762/1/61
ISSN
0004-637X
Volume
762
Issue
1
Page Count
11
Article Number
61
Keyword(s)
Astronomy & Astrophysics, magnetic fields, stars: individual (Swift J1626.6-5156), stars: neutron, X-rays: binaries, PULSE PHASE SPECTROSCOPY, LONG-TERM VARIABILITY, TIMING-EXPLORER, VELA X-1, SUZAKU OBSERVATIONS, 2004-2005 OUTBURST, RESOLVED ANALYSIS, CENTAURUS X-3, SPACED DATA, HERCULES-X-1
Citation
DeCesar M, Boyd P, Pottschmidt K, Wilms J, Suchy S, Miller M. THE Be/X-RAY BINARY SWIFT J1626.6-5156 AS A VARIABLE CYCLOTRON LINE SOURCE. ASTROPHYS J. 2013;762 (1):11.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • On any website, arXiv, scientific social networks (except Research Gate) or non-commercial open access repository.
  • Publisher's version/PDF may be used on any website or authors' institutional repository
  • Publisher copyright and source must be acknowledged
  • Must link to publisher version
  • Publisher's version/PDF may be used
  • Authors depositing in arXiv must they choose the first licence statement offered by arXiv when uploading their article – a "non-exclusive licence to distribute"
  • Publisher last contacted on 10/02/2016

More usage information may be available at SHERPA/RoMEO