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The X-ray pulse profile of BG CMi

โœ Scribed by Chul-Sung Choi; Tadayasu Dotani; Yonggi Kim; Dongsu Ryu


Publisher
Elsevier Science
Year
2007
Tongue
English
Weight
368 KB
Volume
12
Category
Article
ISSN
1384-1076

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โœฆ Synopsis


We present an analysis of the X-ray data of a magnetic cataclysmic variable, BG CMi, obtained with ROSAT in March 1992 and with ASCA in April 1996. We show that four peaks clearly exist in the X-ray pulse profile, unlike a single peak found in the optical profile. The fluxes of two major pulses are $2-5 times larger than those of two minor pulses. The fraction of the total pulsed flux increases from 51% to 85% with increasing energy in 0.1-2.0 keV, whereas it decreases from 96% to 22% in 0.8-10 keV. We discuss the implications of our findings for the origin of the pulse profile and its energy dependence.


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