No anticorrelation between cyclotron line energy and X-ray flux in 4U 0115+634

Record Type
Journal Articles
Full Title
No anticorrelation between cyclotron line energy and X-ray flux in 4U 0115+634
Author(s)
Mueller S, Ferrigno C, Kuehnel M, Schoenherr G, Becker P, Wolff M, Hertel D, Schwarm F, Grinberg V, Obst M, Caballero I, Pottschmidt K, Fuerst F, Kreykenbohm I, Rothschild R, Hemphill P, Nunez S, Torrejon J, Klochkov D, Staubert R, Wilms J
Publication Title
ASTRONOMY & ASTROPHYSICS
Publication Title (abbreviated)
ASTRON ASTROPHYS
Publication Date
2013 Mar
DOI
10.1051/0004-6361/201220359
ISSN
0004-6361
Volume
551
Page Count
10
Article Number
A6
Keyword(s)
Astronomy & Astrophysics, X-rays: binaries, pulsars: individual 4U 0115+634, magnetic fields, TIMING-EXPLORER, GIANT OUTBURST, RESONANCE ENERGIES, ABSORPTION FEATURE, PULSAR 4U-0115+63, MAGNETIC-FIELDS, HIGH-RESOLUTION, NEUTRON-STARS, INTEGRAL DATA, EXO 2030+375
Citation
Mueller S, Ferrigno C, Kuehnel M, Schoenherr G, Becker P, Wolff M, Hertel D, Schwarm F, Grinberg V, Obst M, et al. No anticorrelation between cyclotron line energy and X-ray flux in 4U 0115+634. ASTRON ASTROPHYS. 2013;551 10.
Permissions
Copyright 2013 EDP Sciences.
Conditions of Use
  • Author can archive pre-print (i.e., pre-refereeing)
  • Author can archive post-print (i.e., final draft post-refereeing)
  • On author's personal website or institutional website or OAI compliant website
  • Some journals require an embargo for deposit in funder's designated repositories (see journal)
  • Publisher's version/PDF may be used (see journal)
  • Must link to publisher version
  • Publisher copyright and source must be acknowledged
  • Non-commercial

More usage information may be available at SHERPA/RoMEO