Kretschmar P, Keating J, Kreykenbohm I, Wilms J, Staubert R (2010)
Publication Status: Published
Publication Type: Conference contribution
Publication year: 2010
Book Volume: 1248
Pages Range: 167-+
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.
APA:
Kretschmar, P., Keating, J., Kreykenbohm, I., Wilms, J., & Staubert, R. (2010). Long-term variability of Vela X-1. (pp. 167-+).
MLA:
Kretschmar, Peter, et al. "Long-term variability of Vela X-1." 2010. 167-+.
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