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X-ray observations of selected cataclysmic variable stars using the Einstein observatory

Journal Article · · Astrophys. J.; (United States)
DOI:https://doi.org/10.1086/158836· OSTI ID:6295970
X-ray observations of twelve cataclysmic variable stars using the Einstein Observatory are reported. Nine of these stars, representing all subclasses of cataclysmic variables, were detected. Their fluxes range from 2 x 10/sup -13/ to 1 x 10/sup -11/ ergs cm/sup -2/ s/sup -1/ in the energy interval 0.16--4.5 keV. The 2 sigma upper limits for the remaining stars, which include the so-called magnetic rotators DQ Her and V533 Her, are approx.1 x 10/sup -13/ ergs cm/sup -2/ s/sup -1/. The spectra of all the sources detected are relatively hard (kT> or approx. =5 keV). There is no evidence for an ultrasoft emission component (kTapprox.50 eV) such as has been observed from the dwarf novae SS Cyg and U Gem during optical outburst, even though two of the dwarf novae in the sample were in outburst when they were observed. The X-ray and optical fluxes of the objects observed can be understood in terms of differences in mass accretion rate if the accreting stars in these close binary systems possess a weak magnetic field. The X-ray data are also consistent with models of dwarf novae in which only a small portion of the matter transferred from the red star is accreted onto the degenerate dwarf during optical quiescence.
Research Organization:
California Institute of Technology
OSTI ID:
6295970
Journal Information:
Astrophys. J.; (United States), Journal Name: Astrophys. J.; (United States) Vol. 245:2; ISSN ASJOA
Country of Publication:
United States
Language:
English