English
Related papers

Related papers: CSS091109:035759+102943 - a candidate polar

200 papers

We report the discovery of 1RXS J173006.4+033813, a polar cataclysmic variable with a period of 120.21 min. The white dwarf primary has a magnetic field of B = 42+6-5 MG, and the secondary is a M3 dwarf. The system shows highly symmetric…

Solar and Stellar Astrophysics · Physics 2015-05-19 Varun B. Bhalerao , Marten H. van Kerkwijk , Fiona A. Harrison , Mansi M. Kasliwal , S. R. Kulkarni , Vikram R. Rana

The spectrum of the recently discovered cataclysmic variable star (CV) ASAS-SN 13cl shows that a secondary star with spectral type K4 (+- 2 subclasses) contributes roughly half the optical light. The radial velocities of the secondary are…

Solar and Stellar Astrophysics · Physics 2015-06-23 John R. Thorstensen

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

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 present photometry and spectroscopy of HT Camelopardalis, a recently discovered X-ray-bright cataclysmic variable. The spectrum shows bright lines of H, He I, and He II, all moving with a period of 0.059712(1) d, which we interpret as…

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…

High Energy Astrophysical Phenomena · Physics 2025-07-15 Rahul Sharma , Chetana Jain , Biswajit Paul , Anjan Dutta , Vikram Rana

We report on optical spectroscopic and photometric follow-up observations of the eROSITA discovered transient SRGt 062340.2-265751 and show that it displays the characteristics of a nova-like cataclysmic variable (CV), with possible…

We report a spectroscopic orbit with period P = 3.52433 +/- 0.00027 days for the planetary companion that transits the solar-type star HD209458. For the metallicity, mass, and radius of the star we derive [Fe/H] = 0.00 +/- 0.02, M = 1.1 +/-…

We report photometry and spectroscopy of the novalike variable DW Cancri. The spectra show the usual broad H and He emission lines, with an excitation and continuum slope characteristic of a moderately high accretion rate. A radial-velocity…

We present here results of an optical spectroscopic study of a new Cataclysmic Variable SDSS J001856.93+345444.3. We demonstrate that the most probable value of the orbital period of the system is Porb = 0.6051 \pm 0.022 days (=14.5226…

Solar and Stellar Astrophysics · Physics 2010-09-30 D. Gonzalez , G. Tovmassian , S. Zharikov , A. Aviles , J. Echevarria

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…

Solar and Stellar Astrophysics · Physics 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

Twenty-one new optical light curves, including five curves obtained in 2009 and sixteen curves detected from the AAVSO International Database spanning from 1977 to 2011, demonstrate 16 new primary minimum light times in the high state.…

Solar and Stellar Astrophysics · Physics 2013-08-29 Zhibin Dai , Shengbang Qian , Linjia Li

We report the identification and follow-up of the transient SRG 062340.2-265715 detected with both instruments on board the Spektrum-Roentgen-Gamma mission. Optical spectroscopy of the G=12.5 counterpart firmly classifies the object as a…

We report the identification of the cataclysmic variable 1RXSJ062518.2+733433 as an intermediate polar. The orbital period of the system is determined to be 283.0+-2 min from the radial velocity variation of Halpha, measured in an extensive…

Astrophysics · Physics 2009-11-07 S. Araujo-Betancor , B. T. Gaensicke , H. -J. Hagen , P. Rodriguez-Gil , D. Engels

We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXSJ173021.5-055933, together with simultaneous UV and coordinated optical photometry aiming at…

We present modeling of the long-term optical light curve and radial velocity curve of the binary stellar system CXOGBS J175553.2-281633, first detected in X-rays in the \textit{Chandra} Galactic Bulge Survey. We analyzed 7 years of optical…

The growing number of multi-epoch optical and infrared sky surveys are uncovering unprecedented numbers of new variable stars, of an increasing number of types. The short interval between observations in adjacent near infrared filters in…

Solar and Stellar Astrophysics · Physics 2022-06-29 C. Morris , T. J. Maccarone , P. W. Lucas , J. Strader , C. T. Britt , N. Miller , S. J. Swihart , W. J. Cooper , J. E. Drew , Z. Guo

We present photometric and polarimetric observations of a new magnetic cataclysmic variable, presumably a polar, USNO-A2.0 0825-18396733. The photometric observations were carried out with the SAO RAS Zeiss-1000 telescope, and the…

Solar and Stellar Astrophysics · Physics 2017-08-29 V. L. Afanasiev , N. V. Borisov , M. M. Gabdeev

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…

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…