dc.contributor.author | BALMAN, Şölen | |
dc.contributor.author | Sion, Edward M. | |
dc.contributor.author | Godon, Patrick | |
dc.date.accessioned | 2021-03-05T15:56:09Z | |
dc.date.available | 2021-03-05T15:56:09Z | |
dc.date.issued | 2014 | |
dc.identifier.citation | BALMAN Ş., Godon P., Sion E. M. , "SWIFT X-RAY ILLESCOPE OBSERVATIONS OF THE NOVA-LIKE CATACLYSMIC VARIABLES MV Lyr, BZ Cam, AND V592 Cas", ASTROPHYSICAL JOURNAL, cilt.794, 2014 | |
dc.identifier.issn | 0004-637X | |
dc.identifier.other | vv_1032021 | |
dc.identifier.other | av_be31f1fd-9644-46e7-b969-3251b4580868 | |
dc.identifier.uri | http://hdl.handle.net/20.500.12627/126340 | |
dc.identifier.uri | https://doi.org/10.1888/0004-637x/794/1/84 | |
dc.description.abstract | We present a total of similar to 45 ks (3 x 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 x 10(-9) M circle dot 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-rayemitting 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) x 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) similar to 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. | |
dc.language.iso | eng | |
dc.subject | Temel Bilimler (SCI) | |
dc.subject | ASTRONOMİ VE ASTROFİZİK | |
dc.subject | Astronomi ve Astrofizik | |
dc.subject | Fizik | |
dc.subject | Uzay bilimi | |
dc.subject | Temel Bilimler | |
dc.title | SWIFT X-RAY ILLESCOPE OBSERVATIONS OF THE NOVA-LIKE CATACLYSMIC VARIABLES MV Lyr, BZ Cam, AND V592 Cas | |
dc.type | Makale | |
dc.relation.journal | ASTROPHYSICAL JOURNAL | |
dc.contributor.department | Orta Doğu Teknik Üniversitesi , Fen Fakültesi , Astrofizik Ana Bilim Dalı | |
dc.identifier.volume | 794 | |
dc.identifier.issue | 1 | |
dc.contributor.firstauthorID | 2211737 | |