Long-term variability of Vela X-1

Details Long-term variability of Vela X-1 Long-term variability of Vela X-1

Jul 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010aipc.1248..167k&link_type=abstract

X-RAY ASTRONOMY 2009; PRESENT STATUS, MULTI-WAVELENGTH APPROACH AND FUTURE PERSPECTIVES: Proceedings of the International Confer

Astronomy and Astrophysics

Astronomy

X-Ray Pulsars, X-Ray Binary Stars, Stellar Winds, Accretion Disks, Pulsars, X-Ray Binaries, Mass Loss And Stellar Winds, Accretion And Accretion Disks

Scientific paper

The archetypical wind-accreting X-ray pulsar Vela X-1 is known to be
variable on a large range of timescales. Relatively tranquil phases
exist as well as extended phases of high variability and flaring. We
present results from a systematic study of variations with orbital phase
and other timescales based on RXTE/ASM and Swift/BAT data.

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