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Related papers: The Polar CSS 081231:071126+440405 at a Low Accret…

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The eclipsing polar CSS081231 turned bright (V_max ~ 14.5) in late 2008 and was subsequently observed intensively with small and medium-sized telescopes. A homogeneous analysis of this comprehensive dataset comprising 109 eclipse epochs is…

Solar and Stellar Astrophysics · Physics 2015-06-23 A. D. Schwope , F. Mackebrandt , B. D. Thinius , C. Littlefield , P. Garnavich , A. Oksanen , T. Granzer

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 describe briefly the properties of the recently completed Southern African Large Telescope (SALT), along with its first light imager SALTICAM. Using this instrument, we present 4.3 hr of high speed unfiltered photometric observations of…

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 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…

High Energy Astrophysical Phenomena · Physics 2025-10-22 V. Yu. Kochkina , A. I. Kolbin , T. A. Fatkhullin , A. S. Vinokurov , N. V. Borisov

We analyze spectroscopic and photometric observations of the eclipsing polar BS Tri. The polar's light curve shape variations can be interpreted by changing contributions of the accretion stream to the integral radiation of the system.…

High Energy Astrophysical Phenomena · Physics 2022-12-26 A. I. Kolbin , N. V. Borisov , N. A. Serebriakova , V. V. Shimansky , N. A. Katysheva , M. M. Gabdeev , S. Yu. Shugarov

We report the discovery of a new eclipsing polar, CRTS J035010.7+323230 (hereafter CRTS J0350+3232). We identified this cataclysmic variable (CV) candidate as a possible polar from its multi-year Catalina Real-Time Transient Survey (CRTS)…

Solar and Stellar Astrophysics · Physics 2019-07-31 Paul A. Mason , Natalie K. Wells , Mokhine Motsoaledi , Paula Szkody , Emmanuel Gonzalez

We report the analysis of time-series of optical photometry of SDSS J0926+3624 collected with the Liverpool Robotic Telescope between 2012 February and March while the object was in quiescence. We combined our median eclipse timing with…

Solar and Stellar Astrophysics · Physics 2018-05-24 Wagner Schlindwein , Raymundo Baptista

We report the discovery of a new, bright (V = 17 mag) AM Her system as the optical counterpart of the soft ROSAT All-Sky-Survey source RX J1846.9+5538 (= 1RXS J184659.4+553834). Optical photometric and spectroscopic follow-up observations…

Astrophysics · Physics 2009-11-07 R. Schwarz , J. Greiner , G. H. Tovmassian , S. V. Zharikov , W. Wenzel

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…

We report the discovery of a bright (V ~ 15), eclipsing, two-pole accreting magnetic cataclysmic variable (CV), a polar, as counterpart of the eROSITA and Gaia transients eRASSt 192932.9-560346 and Gaia21bxo. Frequent large amplitude…

Solar and Stellar Astrophysics · Physics 2022-05-18 Axel Schwope , David A. H. Buckley , Adam Malyali , Stephen Potter , Ole König , Riccardo Arcodia , Mariusz Gromadzki , Arne Rau

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…

Astrophysics · Physics 2016-08-30 Stephen B. Potter , Thomas Augusteijn , Claus Tappert

Based on multiyear INTEGRAL observations of SS433 in 2003-2011, a composite IBIS/ISGRI 18-60 keV orbital light curve is constructed around zero precessional phases psi_{pr}= 0 at the maximim accretion disk opening angle. It shows a peculiar…

High Energy Astrophysical Phenomena · Physics 2013-10-24 A. M. Cherepashchuk , R. A. Sunyaev , S. V. Molkov , E. A. Antokhina , K. A. Postnov , A. I. Bogomazov

The eclipsing low-mass X-ray binary 4U is the prototypical accretion disk corona (ADC) system. We have obtained new time-resolved UV spectrograms of 4U with the Hubble Space Telescope and new V- and J-band light curves with the 1.3-m SMARTS…

Astrophysics · Physics 2009-06-23 A. J. Bayless , E. L. Robinson , R. I. Hynes , T. A. Ashcraft , M. E. Cornell

We present results of optical and infrared photometric monitoring of the eclipsing low-mass X-ray binary V395 Car (2S 0921-630). Our observations reveal a clear, repeating orbital modulation with an amplitude of about one magnitude in B,…

High Energy Astrophysical Phenomena · Physics 2015-06-05 Teresa A. Ashcraft , Robert I. Hynes , Edward L. Robinson

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…

We report time-resolved VR-band CCD photometry of the eclipsing binary RZ Cas obtained with 38-cm Cassegrain telescope at the Crimean Astrophysical Observatory during July 2004 - October 2005. Obtained lightcurves clearly demonstrates rapid…

Astrophysics · Physics 2007-12-13 A. Golovin , E. Pavlenko

We present the first high time resolution light curves for six eclipses of the magnetic cataclysmic variable EP Dra, taken using the superconducting tunnel junction imager S-Cam2. The system shows a varying eclipse profile between…

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 results from six years of recalibrated and new spectropolarimetric data taken with the University of Wisconsin's Half-Wave Spectropolarimeter (HPOL) and six years of new data taken with the photoelastic modulating polarimeter…

Solar and Stellar Astrophysics · Physics 2015-05-30 Jamie R. Lomax , Jennifer L. Hoffman , Nicholas M. Elias , Fabienne A. Bastien , Bruce D. Holenstein
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