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Related papers: 2XMMi J225036.9+573154 - a new eclipsing AM Her bi…

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We report the serendipituous discovery of the new eclipsing polar 2XMMp J131223.4+173659. Its striking X-ray light curve attracted immediate interest when we were visually inspecting the source products of the 2XMMp catalogue. This light…

Astrophysics · Physics 2009-11-13 J. Vogel , K. Byckling , A. Schwope , J. P. Osborne , R. Schwarz , M. G. Watson

We present X-ray and optical data of the newly discovered AM Her variable RX J1802.1+1804 = V884 Her. This X-ray source was observed in the ROSAT All-Sky-Survey in September 1990 and subsequently discovered as a highly variable and soft…

Astrophysics · Physics 2007-05-23 J. Greiner , R. A. Remillard , C. Motch

In this study, we report a discovery from XMM-Newton, which involves the identification and subsequent examination of a newly discovered polar-type cataclysmic variable named XMM J152737.4-205305.9. The discovery was made by matching the…

High Energy Astrophysical Phenomena · Physics 2024-06-12 Samet Ok , Axel Schwope , David A. H. Buckley , Jaco Brink

The hard X-ray source 2PBC J0658.0-1746 was proposed as an eclipsing magnetic cataclysmic variable of the polar type, based on optical follow-ups. We present the first spectral and timing analysis at X-ray energies with XMM-Newton,…

High Energy Astrophysical Phenomena · Physics 2019-07-24 F. Bernardini , D. de Martino , K. Mukai , M. Falanga , N. Masetti

The cataclysmic variable SDSSJ 015543.40+002807.2 is confirmed to be a magnetic system of the AM Herculis type. With an orbital period of 87.13 min, it is also the shortest-period eclipsing Polar known. Monitoring with XMM-Newton finds a…

We report the discovery of a new AM Herculis binary (polar) as the optical counterpart of the soft X-ray source RX J1724.0+4114 detected during the ROSAT all-sky survey. The magnetic nature of this V~17 mag object is confirmed by…

Astrophysics · Physics 2009-10-30 Jochen Greiner , Robert Schwarz , Wolfgang Wenzel

We report on 2MASS J01542930+0053266, a faint eclipsing system composed of two M dwarfs. The variability of this system was originally discovered during a pilot study of the 2MASS Calibration Point Source Working Database. Additional…

We report follow-up XMM-Newton and optical observations of three new polars found in the Sloan Digital Sky Survey. Simple modeling of the X-ray spectra, and consideration of the details of the X-ray and optical lightcurves corroborate the…

We report the results from a detailed analysis of an archival XMM-Newton observation of the X-ray source XGPS-I J183251-100106, which has been suggested as a promising magnetic cataclysmic variable candidate based on its optical properties.…

High Energy Astrophysical Phenomena · Physics 2015-06-11 C. Y. Hui , K. A. Seo , C. P. Hu , L. C. C. Lin , Y. Chou

We have discovered a new AM Her system as the optical counterpart of the ROSAT All-Sky-Survey source RX J1016.9-4103 (= 1RXS J101659.4-410332). The X-ray spectrum is very soft and the X-ray intensity is strongly modulated with the orbital…

Astrophysics · Physics 2007-05-23 Jochen Greiner , Robert Schwarz

A new magnetic cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557. The emission lines show radial velocity variations with a period of 98.2 min. This coincides with the period of deep eclipses (up to 4…

We present low--medium resolution optical spectroscopy of the eclipsing AM Her system MN Hya (RX J0929--24). We determine the magnetic field strength at the primary accretion region of the white dwarf to be 42MG from the spacing of…

Astrophysics · Physics 2009-10-30 G. Ramsay , P. J. Wheatley

We report on the X-ray observations of the eclipsing polar HY Eri (RX J0501-0359), along with its photometric, spectrophotometric, and spectropolarimetric optical variations, collected over 30 years. With an orbital period of 2.855 h, HY…

Solar and Stellar Astrophysics · Physics 2020-02-12 K. Beuermann , V. Burwitz , K. Reinsch , A. Schwope , H. -C. Thomas

We report the discovery of an eclipsing X-ray binary in M101, the first such system to be discovered outside the Local Group. Based on a sequence of 25 Chandra observations that sample a wide range of orbital phases, we find a period of…

Astrophysics · Physics 2008-11-26 Jifeng Liu , Rosanne di Stefano , Jeffrey McClintock , Albert Kong , Joel Bregman , Kip Kuntz

We discovered eclipses and dips in two luminous (and highly variable) X-ray sources in M\,51. One (CXOM51 J132943.3$+$471135) is an ultraluminous supersoft source, with a thermal spectrum at a temperature of about 0.1 keV and characteristic…

High Energy Astrophysical Phenomena · Physics 2018-04-25 Song Wang , Roberto Soria , Ryan Urquhart , Jifeng Liu

Aims: We aim to study the temporal and spectral behaviour of the eclipsing polar CSS081231:071126+440405 from the infrared to the X-ray regime. Methods: We obtained phase-resolved XMM-Newton X-ray observations on two occasions in 2012 and…

High Energy Astrophysical Phenomena · Physics 2015-11-17 H. Worpel , A. D. Schwope

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…

Swift J2218.4+1925, a hard X-ray source detected by Swift BAT, has been proposed as a candidate magnetic cataclysmic variable of the polar type from optical spectroscopy. Using XMM-Newton we perform detailed timing and spectral analysis…

High Energy Astrophysical Phenomena · Physics 2015-06-22 Federico Bernardini , Domitilla de Martino , Koji Mukai , Maurizio Falanga

We report the discovery of a new eclipsing polar, MASTER OT J061451.70-272535.5, detected as an optical transient by MASTER auto-detection software at the recently commissioned MASTER-SAAO telescope. Time resolved (10-20 s) photometry with…

We present XMM-Newton observations of the eclipsing polar EP Dra which cover nearly 3 binary orbital cycles. The X-ray and UV data show evidence for a prominent dip before the eclipse which is due to the accretion stream obscuring the…

Astrophysics · Physics 2009-11-10 Gavin Ramsay , C. M. Bridge , Mark Cropper , K. O. Mason , F. A. Cordova , W. Priedhorsky
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