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We report the discovery of SRGE J075818-612027, a deep stream-eclipsing magnetic cataclysmic variable found serendipitously in SRG/eROSITA CalPV observations of the open cluster NGC~2516 as an unrelated X-ray source. An X-ray timing and…

太阳与恒星天体物理 · 物理学 2023-05-09 Samet Ok , Georg Lamer , Axel Schwope , David A. H. Buckley , Jaco Brink , Jan Kurpas , Dusán Tubín , Iris Traulsen

We present a low-resolution discovery spectrum and CCD-photometry of the bright X-ray source 1RXS J012851.9-233931 found in the ROSAT All-Sky Survey. These first observations suggest that the source is an AM Herculis star (polar) accreting…

天体物理学 · 物理学 2007-05-23 A. D. Schwope , R. Schwarz , J. Greiner

In course of the search for the optical identifications associated with ROSAT X-ray sources we have found a highly variable object with the very unusual long-term behavior, color indices and high X-ray-to-optical flux ratio. We report the…

太阳与恒星天体物理 · 物理学 2015-05-28 D. V. Denisenko , A. J. Drake , S. G. Djorgovski , T. V. Kryachko , A. V. Samokhvalov , A. Yu. Tkachenko

RXJ 0501.7-0359 is a new V ~ 17 mag eclipsing polar discovered during the ROSAT all-sky survey (RASS). Extensive follow-up observations at X-ray (pointed ROSAT PSPC and HRI observations) and optical (time-resolved photometry and…

天体物理学 · 物理学 2007-05-23 Vadim Burwitz , Klaus Reinsch , Klaus Beuermann , Hans-Christoph Thomas

A new cataclysmic variable is identified as the optical counterpart of the faint and hard X-ray source RX J0757.0+6306 discovered during the ROSAT all-sky survey. Strong double-peaked emission lines bear evidence of an accretion disc via an…

We report the discovery of a new catacysmic variable system, RXJ051541+0104.6. The optical spectrum has a blue continuum with superposed H~I and He~I and II emission lines. The soft X-ray spectrum is well fit with a 50~eV black body. The…

天体物理学 · 物理学 2009-10-22 F. M. Walter , S. J. Wolk , N. R. Adams

We aimed to identify the variable X-ray source 3XMM J000511.8+634018, which was serendipitously discovered through routine inspections while the 3XMM catalogue was compiled. We analysed the archival XMM-Newton observation of the source,…

太阳与恒星天体物理 · 物理学 2020-05-13 A. D. Schwope , H. Worpel , N. A. Webb , F. Koliopanos , S. Guillot

We report optical and X-ray observations of the high-field polar RXJ1007.5-2017 performed between 1990 and 2012. It has an orbital period of 208.60 min determined from the ellipsoidal modulation of the secondary star in an extended low…

高能天体物理现象 · 物理学 2015-06-11 H. -C. Thomas , K. Beuermann , K. Reinsch , A. D. Schwope , V. Burwitz

We report on XMM-Newton and NuSTAR X-ray observations of the prototypical polar, AM Herculis, supported by ground-based photometry and spectroscopy, all obtained in high accretion states. In 2005, AM Herculis was in its regular mode of…

太阳与恒星天体物理 · 物理学 2020-10-14 A. D. Schwope , H. Worpel , I. Traulsen , D. Sablowski

The transient optical source MASTER OT J072007.30+451611.6 has been recently discovered and proposed as a peculiar polar with an unusually high amplitude of the orbital brightness variation in the optical of $\sim$3 mag. To clarify its…

This study confirms MLS110213:022733+130617 as a new eclipsing polar. We performed optical spectroscopic, polarimetric and photometric follow-up of this variable source identified by the Catalina Real Time Transient Survey. Using the…

太阳与恒星天体物理 · 物理学 2015-05-14 K. M. G Silva , C. V. Rodrigues , A. S. Oliveira , L. A. Almeida , D. Cieslinski , J. E. R. Costa , F. J. Jablonski

We have analyzed phase-resolved photometric and spectroscopic observations of the eclipsing polar SDSS J002637.06+242915.6. The light curve has a M-shaped bright phase that was reproduced using a simple model of an accreting magnetic white…

高能天体物理现象 · 物理学 2025-10-22 V. Yu. Kochkina , A. I. Kolbin , T. A. Fatkhullin , A. S. Vinokurov , N. V. Borisov

We present photometric and spectroscopic observations of the cataclysmic variable MASTER OT J132104.04+560957.8 which strongly indicate that it is a polar with an orbital period of 91 minutes. The optical light curve shows two maxima and…

太阳与恒星天体物理 · 物理学 2014-12-30 Colin Littlefield , Peter Garnavich , Katrina Magno , Marc Murison , Shanel Deal , Colin McClelland , Benjamin Rose

We present optical photometric and spectroscopic observations, and an analysis of archival X-ray data of three polars: RX J0859.1+0537, RX J0749.1-0549, and RX J0649.8-0737. Optical light curves of these three polars reveal eclipse features…

太阳与恒星天体物理 · 物理学 2020-01-08 Arti Joshi , J. C. Pandey , Ashish Raj , K. P. Singh , G. C. Anupama , H. P. Singh

We report photopolarimetric observations of a new eclipsing polar (AM Herculis system) discovered in the Calan-Tololo survey. The photometry and polarimetry are modulated on a period of ~101 minutes. Circular polarization variations are…

天体物理学 · 物理学 2016-08-30 Stephen B. Potter , Thomas Augusteijn , Claus Tappert

We present phase-resolved spectral and multicolor CCD-photometric observations of the eclipsing polar RX J0719.2+6557 obtained with relatively high time (~600 sec/15 sec) and spectral (2.1 A) resolution when the system was in a high…

The detection and characterization of periodic X-ray signals are crucial for identifying new compact objects and studying the mechanisms powering their emission. We report on the timing and spectral variability of CXOU J204734.8+300105, a…

高能天体物理现象 · 物理学 2025-07-15 Rahul Sharma , Chetana Jain , Biswajit Paul , Anjan Dutta , Vikram Rana

We present phase-resolved spectroscopy and photometry of a source discovered with the Chandra Galactic Bulge Survey (GBS), CXOGBSJ174444.7-260330 (aka CX93 and CX153 in the previously published GBS list). We find two possible values for the…

Optical and X-ray observations suggested that the 9.38 h binary, SWIFT J0746.3- 1608 could be a Cataclysmic Variable of the magnetic or nova-like type, or a low mass X-ray binary. Its optical, UV, and X-ray light curves are strongly…

高能天体物理现象 · 物理学 2019-01-09 F. Bernardini , D. de Martino , K. Mukai , M. Falanga

We report the discovery of 1RXH J082623.6-505741, a 10.4 hr orbital period compact binary. Modeling extensive optical photometry and spectroscopy reveals a $\sim 0.4 M_{\odot}$ K-type secondary transferring mass through a low-state…