Pulse phase-resolved X-ray spectroscopy of the transient high-mass X-ray binary V 0332 + 53

Details Pulse phase-resolved X-ray spectroscopy of the transient high-mass X-ray binary V 0332 + 53 Pulse phase-resolved X-ray spectroscopy of the transient high-mass X-ray binary V 0332 + 53

Jun 1992

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992mnras.256..725u&link_type=abstract

Monthly Notices of the Royal Astronomical Society (ISSN 0035-8711), vol. 256, no. 4, June 15, 1992, p. 725-735. Research support

Astronomy and Astrophysics

Astronomy

9

Pulsars, Spectrum Analysis, X Ray Binaries, X Ray Spectroscopy, Astronomical Models, Exosat Satellite

Scientific paper

An analysis is conducted of Exosat observations of the transient binary X-ray pulsar V 0332 + 53 during a series of flares, which yielded simultaneous high energy and time resolutions. The results obtained are interpreted in terms of a system in which the line-of-sight from the earth is not close to the magnetic axis of the neutron star, and in which contributions from two active regions vary as the outburst evolves.

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