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Related papers: On the space density of X-ray selected cataclysmic…

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We use the ROSAT North Ecliptic Pole (NEP) survey to construct a small, but purely X-ray flux-limited sample of cataclysmic variable stars (CVs). The sample includes only 4 systems, 2 of which (RX J1715.6+6856 and RX J1831.7+6511) are new…

Astrophysics · Physics 2009-11-13 M. L. Pretorius , C. Knigge , D. O'Donoghue , J. P. Henry , I. M. Gioia , C. R. Mullis

We present constraints on the space densities of both non-magnetic and magnetic cataclysmic variables, and discuss some implications for models of the evolution of CVs. The high predicted non-magnetic CV space density is only consistent…

Solar and Stellar Astrophysics · Physics 2014-07-14 Magaretha L. Pretorius

We present the first volume-limited sample of cataclysmic variables (CVs), selected using the accurate parallaxes provided by the second data release (DR2) of the ESA $\mathit{Gaia}$ space mission. The sample is composed of 42 CVs within…

We present volume-limited samples of cataclysmic variables (CVs) and AM CVn binaries jointly selected from SRG/eROSITA eRASS1 and \textit{Gaia} DR3 using an X-ray + optical color-color diagram (the ``X-ray Main Sequence"). This tool…

The spatial distribution, Galactic model parameters and luminosity function of cataclysmic variables (CVs) are established using re-estimated trigonometric parallaxes of {\it Gaia} DR3. The data sample of 1,587 CVs in this study is claimed…

Solar and Stellar Astrophysics · Physics 2023-03-29 R. Canbay , S. Bilir , A. Özdönmez , T. Ak

Cataclysmic variables (CVs) are the most numerous population among the Galactic objects emitting in hard X-rays. Most probably, they are responsible for the extended hard X-ray emission of the Galactic ridge and the central Galactic…

High Energy Astrophysical Phenomena · Physics 2022-02-23 Valery F. Suleimanov , Victor Doroshenko , Klaus Werner

We combine two complete, X-ray flux-limited surveys, the ROSAT Bright Survey (RBS) and the ROSAT North Ecliptic Pole (NEP) survey, to measure the space density (\rho) and X-ray luminosity function (\Phi) of non-magnetic CVs. The combined…

Solar and Stellar Astrophysics · Physics 2015-05-30 Magaretha L. Pretorius , Christian Knigge

We use the complete, X-ray flux-limited ROSAT Bright Survey (RBS) to measure the space density of magnetic cataclysmic variables (mCVs). The survey provides complete optical identification of all sources with count rate >0.2/s over half the…

Solar and Stellar Astrophysics · Physics 2015-06-15 Magaretha L. Pretorius , Christian Knigge , Axel D. Schwope

(abridged) We present an account of known cataclysmic variables (CVs) that were detected as X-ray sources in eROSITA X-ray surveys and have Gaia DR3 counterparts. We address standard CVs with main sequence donors and white dwarfs accreting…

Solar and Stellar Astrophysics · Physics 2024-07-31 Axel Schwope , Kira Knauff , Jan Kurpas , Mara Salvato , Beate Stelzer , Laurent Stütz , Dusan Tubín-Arenas

We present a sample of eight cataclysmic variables (CVs) identified among the X-ray sources of the 400 square degree (400d) X-ray ROSAT/PSPC survey. Based on this sample, we have obtained preliminary constraints on the X-ray luminosity…

High Energy Astrophysical Phenomena · Physics 2017-01-18 R. Burenin , M. Revnivtsev , A. Tkachenko , V. Vorobyev , A. Semena , A. Meshcheryakov , S. Dodonov , M. Eselevich , M. Pavlinsky

We present a sample of cataclysmic variables (CVs) identified among the X-ray sources from the 400 square degree X-ray survey based on ROSAT pointing data (400d). The procedure of the CV selection among the X-ray sources using additional…

The spatial distribution, galactic model parameters and luminosity function of cataclysmic variables (CVs) in the solar neighbourhood have been determined from a carefully established sample of 459 CVs. The sample contains all of the CVs…

Astrophysics · Physics 2008-11-26 T. Ak , S. Bilir , S. Ak , Z. Eker

We measure the spatial distribution and hard X-ray luminosity function of cataclysmic variables (CVs) using the INTEGRAL all-sky survey in the 17-60 keV energy band. The vast majority of the INTEGRAL detected CVs are intermediate polars…

Astrophysics · Physics 2009-11-13 M. Revnivtsev , S. Sazonov , R. Krivonos , H. Ritter , R. Sunyaev

By studying Swift X-ray spectra of an optically-selected, non-magnetic sample of nearby cataclysmic variables (CVs), we show that there is a population with X-ray luminosity much lower than accounted for in existing studies. We find an…

High Energy Astrophysical Phenomena · Physics 2015-06-12 R. C. Reis , P. J. Wheatley , B. T. Gansicke , J. P. Osborne

Cataclysmic variables (CVs) are binary systems with a white dwarf accreting matter from a low-mass star, making them significant sources of X-ray emission in the Galaxy. We present a systematic search for X-ray emitting CV candidates by…

Instrumentation and Methods for Astrophysics · Physics 2025-06-25 Xiangxiang Wang , Jumpei Takata

In order to determine the spatial distribution, Galactic model parameters and luminosity function of cataclysmic variables (CVs), a $J$-band magnitude limited sample of 263 CVs has been established using a newly constructed…

Astrophysics of Galaxies · Physics 2015-06-22 A. Ozdonmez , T. Ak , S. Bilir

We compare the X-ray spectra and luminosities, in the 2-8 keV band, of known and suspected cataclysmic variables (CVs) in different environments, assessing the nature of these source populations. These objects include nearby CVs observed…

Astrophysics · Physics 2009-06-23 Craig O. Heinke , Ashley J. Ruiter , Michael P. Muno , Krzysztof Belczynski

A personal selection of noteworthy X-ray results on CVs are presented, with emphasis on XMM-Newton and Chandra observations. Progressing roughly from broad-band view to narrow-band, high spectral resolution studies, I summarize: the energy…

Astrophysics · Physics 2007-05-23 K. Mukai

We present 855 cataclysmic variable candidates detected by the Catalina Real-time Transient Survey (CRTS) of which at least 137 have been spectroscopically confirmed and 705 are new discoveries. The sources were identified from the analysis…

We give an identification summary and results of polarimetric, photometric and spectroscopic follow-up observations of new, X-ray bright cataclysmic variables. These were identified as optical counterparts of high galactic latitude sources…

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