-X-Ray Observations of the Nova-like Cataclysmic Variables MV Lyr, BZ Cam, and V592 Cas
Aug 8, 201412 pages
Published in:
- Astrophys.J. 794 (2014) 1, 84
- Published: Sep 25, 2014
e-Print:
- 1408.1996 [astro-ph.HE]
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Abstract: (IOP)
We present a total of ~45 ks (3 × 15 ks) of Swift X-Ray Telescope (XRT) observations for three nonmagnetic nova-like (NL) cataclysmic variables (CVs, MV Lyr, BZ Cam, V592 Cas) in order to study characteristics of boundary layers (BLs) in CVs. The nonmagnetic NLs are found mostly in a state of high mass accretion rate (≥1 × 10(–)(9) M (☉) yr(–)(1)), and some show occasional low states. Using the XRT data, we find optically thin multiple-temperature cooling flow type emission spectra with X-ray temperatures (kT (max)) of 21-50 keV. These hard X-ray-emitting BLs diverge from simple isobaric cooling flows, indicating X-ray temperatures that are of virial values in the disk. In addition, we detect power-law emission components from MV Lyr and BZ Cam and plausibly from V592 Cas, which may be a result of the Compton scattering of the optically thin emission from the fast wind outflows in these systems and/or Compton upscattering of the soft disk photons. The X-ray luminosities of the (multitemperature) thermal plasma emission in the 0.1-50.0 keV range are (0.9-5.0) × 10(32) erg s(–)(1). The ratio of the X-ray and disk luminosities (calculated from the UV-optical wavelengths) yields an efficiency (L(x) /L (disk)) ~ 0.01-0.001. Given this non-radiative ratio for the X-ray-emitting BLs with no significant optically thick blackbody emission in the soft X-rays (consistent with ROSAT observations), together with the high/virial X-ray temperatures, we suggest that high-state NL systems may have optically thin BLs merged with ADAF-like flows and/or X-ray coronae. In addition, we note that the axisymmetric bipolar and/or rotation-dominated fast-wind outflows detected in these three NLs (particularly BZ Cam and V592 Cas) or some other NL may also be explained in the context of ADAF-like BL regions.Note:
- 36 pages, 3 tables, 4 figures; Astrophysical Journal in PRESS
- accretion, accretion disks
- binaries: close
- novae, cataclysmic variables
- white dwarfs
- X-rays: individual
References(123)
Figures(6)
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