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Related papers: X-ray Emission from Magnetic Cataclysmic Variables

200 papers

W2 (CXOGlb J002415.8-720436) is a cataclysmic variable (CV) in the Galactic globular cluster 47 Tucanae. Its modulation was discovered within the CATS@BAR project. The source shows all the properties of magnetic CVs, but whether it is a…

High Energy Astrophysical Phenomena · Physics 2024-09-18 R. Amato , N. La Palombara , M. Imbrogno , G. L. Israel , P. Esposito , D. de Martino , N. A. Webb , R. Iaria

The X-ray source RX J2015.6+3711 was discovered by ROSAT in 1996 and recently proposed to be a cataclysmic variable (CV). Here we report on an XMM-Newton observation of RX J2015.6+3711 performed in 2014, where we detected a coherent X-ray…

High Energy Astrophysical Phenomena · Physics 2021-01-27 Francesco Coti Zelati , Nanda Rea , Sergio Campana , Domitilla De Martino , Alessandro Papitto , Samar Safi-Harb , Diego F. Torres

Spiral density waves are thought to be excited in the accretion discs of accreting compact objects, including Cataclysmic Variable stars (CVs). Observational evidence has been obtained for a handful of systems in outburst over the last two…

High Energy Astrophysical Phenomena · Physics 2019-11-06 R. Ruiz-Carmona , P. J. Groot , D. T. H. Steeghs

ASCA and GINGA X-ray data from the magnetic Cataclysmic Variable BY Cam show that the spectrum is strongly affected by complex absorption, probably from the pre-shock accretion column. The intrinsic emission from the shock is significantly…

Astrophysics · Physics 2015-06-24 C. Done , P. Magdziarz

We compare some of the properties of rapid oscillations in cataclysmic variables and X-Ray binaries. In addition to the earlier recognition that both types possess the same correlation between high and low frequency quasi-periodic…

Astrophysics · Physics 2009-11-10 Brian Warner , Patrick A. Woudt

Radiation of X-ray bursts and of accretion shocks in weakly magnetized neutron stars in low-mass X-ray binaries is produced in plane-parallel atmospheres dominated by electron scattering. We first discuss polarization produced by single…

High Energy Astrophysical Phenomena · Physics 2016-06-01 Juri Poutanen

Thanks to aggressive campaigns of multi-wavelength observations of X-ray binaries in outbursts over the last decade or so, we have now reached a reasonable understanding of their radio phenomenology in response to changes in the global…

Astrophysics · Physics 2009-04-14 Elena Gallo

Bipolar outflows are present in many disk-accreting astrophysical systems. In disk-accreting cataclysmic variables (CVs), these outflows are responsible for most of the strong features in the ultraviolet spectra of these systems. However,…

Astrophysics · Physics 2009-11-07 Knox S. Long , Christian Knigge

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…

The analysis of the third INTEGRAL/IBIS survey has revealed several new cataclysmic variables, most of which turned out to be intermediate polars, thus confirming that these objects are strong emitters in hard X-rays. Here we present high…

Astrophysics · Physics 2009-11-13 R. Landi , L. Bassani , A. J. Dean , A. J. Bird , M. Fiocchi , A. Bazzano , J. A. Nousek , J. P. Osborne

We report on the properties of 71 known cataclysmic variables (CVs) in photometric Halpha emission line surveys. Our study is motivated by the fact that the Isaac Newton Telescope (INT) Photometric Halpha Survey of the northern galactic…

Cataclysmic variable (CVs) are close interacting binaries in which a white dwarf accretes materials from a low mass main sequence companion. CVs can experience nova eruptions due to low mass transfer rates. In the standard theory of CV…

Solar and Stellar Astrophysics · Physics 2025-07-31 Wenshi Tang , Xiangdong Li , Bo Wang

We resume the discussion about irradiation-driven mass transfer cycles in semi- detached compact binary systems. The analytical model that describes the onset of these cycles, which occur on a thermal timescale of the donor star, is…

Astrophysics · Physics 2009-11-10 A. Büning , H. Ritter

Recent spectroscopic observations have identified several cataclysmic variables non-solar metal abundances. We present theoretical models which examine the level of core evolution expected for CV secondaries prior to contact. Our results…

Astrophysics · Physics 2015-06-24 Steve B. Howell

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 present our analysis of new and archived observations of two candidate magnetic cataclysmic variables, namely 1RXS J174320.1-042953 and YY Sex. 1RXS J174320.1-042953 was observed in two distinctive high and low states where a phase shift…

High Energy Astrophysical Phenomena · Physics 2023-03-01 Nikita Rawat , J. C. Pandey , Arti Joshi , Stephen B. Potter , Alisher S. Hojaev , Michaël De Becker , Srinivas M Rao , Umesh Yadava

We report on the discovery of two new faint cataclysmic variables. The objects were selected as candidates from two different imaging surveys aimed at the discovery of such faint systems. One survey used color and variability while the…

Astrophysics · Physics 2009-11-07 S. B. Howell , E. Mason , M. Huber , R. Clowes

In this paper the current status of high-energy research on the hard X-ray characteristics of the persistent emission from magnetars is reviewed. Focus is put on recent intriguing results for 1RXS J1708-40, from phase resolved spectral…

Astrophysics · Physics 2008-10-28 L. Kuiper , P. R. den Hartog , W. Hermsen

The Catalog and Atlas of Cataclysmic Variables (Edition 1 - 1993) and Edition 2 - 1997) has been a valuable source of information for the cataclysmic variable (CV) community. However, the goal of having a central location for all objects is…

Astrophysics · Physics 2009-11-06 R. A. Downes , R. F. Webbink , M. M. Shara , Hans Ritter , Ulrich Kolb , Hilmar W. Duerbeck

The properties of X-ray emission from accreting black holes are reviewed. The contemporary observational picture and current status of theoretical understanding of accretion and formation of X-ray radiation in the vicinity of the compact…

High Energy Astrophysical Phenomena · Physics 2014-11-20 M. Gilfanov