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Using the Hubble space Telescope Fine Guidance Sensor, we have measured the trigonometric parallax of the bright cataclysmic variable 1223 Sgr. The absolute parallax is pi(abs)= 1.96+-0.18mas, making V1223 Sgr the most distant CV with a…

天体物理学 · 物理学 2009-11-10 K. Beuermann , Th. E. Harrison , B. E. McArthur , G. F. Benedict , B. T. Gaensicke

GY Cnc is a deeply eclipsing cataclysmic variable star with an orbital period of 4.21 hours that has shown several dwarf nova outbursts. The variable was continuously observed by the K2/Kepler satellite with a short cadence in Campaign 5…

We study the variability of the cataclysmic variable DO Dra, on time-scales of between minutes and decades. The characteristic decay time dt/dm=0.902(3) days/mag was estimated from our 3 nights of CCD R observations. The quiescent data show…

天体物理学 · 物理学 2008-06-13 I. L. Andronov , L. L. Chinarova , W. Han , Y. Kim , J. -N. Yoon

We report spectroscopic observations of seven bright southern cataclysmic variable stars, collected on a single two-week observing run using the 1.9-m Radcliffe telescope at the South African Astronomical Observatory. We used radial…

太阳与恒星天体物理 · 物理学 2023-07-18 John R. Thorstensen , Chase K. Alvarado-Anderson , Abigail D. Burrows , Rowan M. Goebel-Bain , David C. Katz

A radial velocity study of the cataclysmic variable ES Dra (PG 1524+622) is presented. ES Dra is found to have an orbital period of 0.17660 \pm 0.00006 d (4.2384 \pm 0.0014 h). The mass-losing secondary star of ES Dra is detectable in the…

太阳与恒星天体物理 · 物理学 2015-05-28 F. A. Ringwald , Kenia Velasco

We report $I$-band photometric observations of the radio-detected M9.5 dwarf BRI 0021-0214, obtained with the Galway Ultra Fast Imager (GUFI) on the 1.8m Vatican Advanced Technology Telescope VATT at Mt. Graham International Observatory,…

太阳与恒星天体物理 · 物理学 2022-11-03 S. Dulaimi , A. Golden , R. P. Boyle , R. F. Butler

We report Johnson's UBVRI photometric and optical spectroscopic observations of a long period variable HP Lyr which up to now has been considered an eclipsing binary with a period of 140 days. The spectral type changes continually from A2-3…

As part of a project to better characterize comparatively bright but so far little studied cataclysmic variables in the southern hemisphere, we have obtained spectroscopic and photometric data of the nova-like variables LS IV -08$^{\rm o}$…

太阳与恒星天体物理 · 物理学 2016-08-26 Albert Bruch , Marcos P. Diaz

Photometric and spectroscopic observations reveal the Sloan Digital Sky Survey cataclysmic variable SDSS J132723.39+652854.2 to be a likely SW Sex star with an orbital period of P = 3.28 hours. The Sloan Digital Sky Survey spectrum shows…

天体物理学 · 物理学 2007-05-23 Michael A. Wolfe , Paula Szkody , Oliver J. Fraser , Lee Homer , Sam Skinner , Nicole M. Silvestri

We find that the ROSAT source 1RXS J105010.3-140431 is a cataclysmic variable with orbital period of 88.6 minutes and a spectrum closely resembling WZ Sge. In particular, emission lines are flanked by Stark-broadened absorption wings…

天体物理学 · 物理学 2009-11-06 R. E. Mennickent , M. Diaz , W. Skidmore , C. Sterken

We announce the identification of a new cataclysmic variable star in the field of the Kepler Mission, KIC J192410.81+445934.9. This system was identified during a search for compact pulsators in the Kepler field. High-speed photometry…

We have obtained simultaneous photometric and spectroscopic observations of the cataclysmic variable 1RXS J064434.5+334451. We have calibrated the spectra for slit losses using the simultaneous photometry allowing to construct reliable…

太阳与恒星天体物理 · 物理学 2016-10-26 J. V. Hernández Santisteban , J. Echevarría , R. Michel , R. Costero

We present the results of spectroscopic-- and orbit--sampled photometric observations of the faint UV-excess object PG 2200+085. The optical CCD photometry observations of this object were performed by the Russian-Turkish 1.5-meter…

天体物理学 · 物理学 2009-11-11 V. Shimansky , N. A. Sakhibullin , I. Bikmaev , H. Ritter , V. Suleimanov , N. Borisov , A. Galeev

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 VLT and Magellan spectroscopy and NTT photometry of nine faint cataclysmic variables (CVs) which were spectroscopically identified by the SDSS. We measure orbital periods for five of these from the velocity variations of the…

This work is dedicated to the discovery of the eclipsing variable star Grigoriev 1 and determining the parameters of its binary system. The star was found through the systematic checking of ultraviolet sources of GALEX space observatory in…

太阳与恒星天体物理 · 物理学 2025-07-02 V. S. Grigoriev , D. V. Denisenko

We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397.Time series photometry was obtained for 30 variable objects. The sample includes 12 new objects, of which 6 show…

天体物理学 · 物理学 2009-11-13 J. Kaluzny , I. B. Thompson , W. Krzeminski

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…

SW Sex stars are an informal sub-class of eclipsing nova-like cataclysmic variables. We report 934 new eclipse times measured over the past 17 years for HS 0728+6738 (V482 Cam), SW Sex, DW UMa, HS 0129+2933 (TT Tri), V1315 Aql, PX And, HS…

太阳与恒星天体物理 · 物理学 2023-07-28 David Boyd

V341 Arae is a 10th-magnitude variable star in the southern hemisphere, discovered over a century ago by Henrietta Leavitt but relatively little studied since then. Although historically considered to be a Cepheid, it is actually blue and…

太阳与恒星天体物理 · 物理学 2018-07-25 Howard E. Bond , Brent Miszalski