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We report detailed follow-up observations of the cataclysmic variable HS2331+3905, identified as an emission-line object in the Hamburg Quasar Survey. An orbital period of 81.08min is unambiguously determined from the detection of eclipses…

We present medium-resolution VLT/FORS2 spectroscopy of six cataclysmic variables discovered by the Sloan Digital Sky Survey. We determine orbital periods for SDSS J023322.61+005059.5 (96.08 +/- 0.09 min), SDSS J091127.36+084140.7 (295.74…

SRGt 062340.2-265751, a cataclysmic variable identified by SRG/eROSITA thanks to its significant X-ray variability, remains poorly characterised despite the multi-wavelength follow-up. We present spectral and timing analyses from the first…

High Energy Astrophysical Phenomena · Physics 2025-12-01 V. A. Cúneo , A. D. Schwope , J. Kurpas , A. Avakyan , J. Brink , D. A. H. Buckley , C. Maitra , M. Veresvarska

We report the detection of Zeeman-split Lalpha absorption pi and sigma+ lines in the far-ultraviolet Hubble Space Telescope/Space Telescope Imaging Spectrograph spectrum of the magnetic cataclysmic variable RX J1554.2+2721. Fitting the STIS…

Astrophysics · Physics 2009-11-10 B. T. Gaensicke , S. Jordan , K. Beuermann , D. de Martino , P. Szkody , T. Marsh , J. Thorstensen

We present results from high speed photometry of a further thirteen faint cataclysmic variables. V356 Aql (Nova Aql 1936) shows flare-like outbursts with recurrence time scales ~ 3000 s, but no coherent periodicities. Aqr1 is an…

Astrophysics · Physics 2009-11-10 Patrick A. Woudt , Brian Warner , Magaretha L. Pretorius

We obtained Calar Alto identification spectra for six cataclysmic variable candidates, and studied archival observations at a range of wavelengths. Two sources were too faint to allow for easy identification by their spectra, and the other…

High Energy Astrophysical Phenomena · Physics 2017-11-08 H. Worpel , A. D. Schwope

We present V and Rc band photometry and optical near-infrared spectroscopy of the cataclysmic variable 1RXS J094432.1+035738. We detected features of a cool secondary star, which can be modeled with a red dwarf of spectral type M2 (+0.5…

We present results from our phase-resolved spectroscopy of the newly identified cataclysmic variable Halpha0242-2802. Halpha0242-2802 was identified from a deep UK Schmidt Halpha-R band survey as a candidate cataclysmic variable. Although…

Astrophysics · Physics 2009-11-11 E. Mason , S. B. Howell

A deep (R ~ 19.5) photographic Halpha Survey of the southern Galactic Plane was recently completed using the UK Schmidt Telescope at the AAO. In addition, we have recently started a similar, CCD-based survey of the northern Galactic Plane…

Astrophysics · Physics 2011-03-10 Andrew Witham , Christian Knigge , Janet Drew , Paul Groot , Robert Greimel , Quentin Parker

W2 (CXOGlb J002415.8-720436) is a cataclysmic variable (CV) in the Galactic globular cluster 47 Tucanae. Its modulation was discovered within the CATS@BAR project. The source shows all the properties of magnetic CVs, but whether it is a…

High Energy Astrophysical Phenomena · Physics 2024-09-18 R. Amato , N. La Palombara , M. Imbrogno , G. L. Israel , P. Esposito , D. de Martino , N. A. Webb , R. Iaria

AE Aqr objects are a class of cataclysmic variable stars in which the rapidly rotating magnetosphere of the white dwarf (WD) primary centrifugally expels most infalling gas before it can accrete onto the WD. The expulsion of the accretion…

Solar and Stellar Astrophysics · Physics 2020-10-02 Colin Littlefield , Peter Garnavich

Studying the population of faint hard X-ray sources along the plane of the Galaxy is challenging because of high-extinction and crowding, which make the identification of individual sources more difficult. IGR J18293-1213 is part of the…

High Energy Astrophysical Phenomena · Physics 2016-06-15 Maïca Clavel , J. A. Tomsick , A. Bodaghee , J. -L. Chiu , F. M. Fornasini , J. Hong , R. Krivonos , G. Ponti , F. Rahoui , D. Stern

The search was performed for cataclysmic variable stars with outlying infrared magnitudes in USNO-B1.0 catalog. The selection was limited to objects in the Northern hemisphere with (B1-R1) < 1 and (R2-I) > 3.5. The search method is…

Solar and Stellar Astrophysics · Physics 2015-05-30 D. V. Denisenko

SDSS-V is carrying out a dedicated survey for white dwarfs, single and in binaries, and we report the analysis of the spectroscopy of 504 cataclysmic variables (CVs) and CV candidates obtained during the first 34 months of observations of…

Two newly identified magnetic cataclysmic variables discovered in the Sloan Digital Sky Survey (SDSS), SDSSJ155331.12+551614.5 and SDSSJ132411.57+032050.5, have spectra showing highly prominent, narrow, strongly polarized cyclotron humps…

The morphology and optical spectrum of IPHASXJ210205+471015, a nebula classified as a possible planetary nebula, are however strikingly similar to those of ATCnc, a classical nova shell around a dwarf nova. To investigate its true nature,…

We present the complete set of thirty four ASCA observations of non-magnetic cataclysmic variables. Timing analysis reveals large X-ray flux variations in dwarf novae in outburst (Z Cam, SS Cyg and SU UMa) and orbital modulation in high…

Astrophysics · Physics 2009-11-10 Darren S. Baskill , Peter J. Wheatley , Julian P. Osborne

Results of photometric and spectroscopic investigations of the recently discovered disc cataclysmic variable star 1RXS J180834.7+101041 are presented. Emission spectra of the system show broad double peaked hydrogen and helium emission…

Solar and Stellar Astrophysics · Physics 2015-05-20 D. G. Yakin , V. F. Suleimanov , V. V. Shimansky , N. V. Borisov , I. F. Bikmaev , N. A. Sakhibullin

The number of discovered non-radially pulsating white dwarfs (WDs) in cataclysmic variables (CVs) is increasing rapidly by the aid of the Sloan Digital Sky Survey (SDSS). We performed photometric observations of two additional objects, SDSS…

Astrophysics · Physics 2007-05-23 R. Nilsson , H. Uthas , M. Ytre-Eide , J-E. Solheim , B. Warner

A new magnetic, eclipsing cataclysmic variable is identified as the counterpart of the X-ray source RX J0719.2+6557 detected during the ROSAT all-sky survey. The relative phasing of photometric and spectroscopic periods indicates a…

Astrophysics · Physics 2007-05-23 G. Tovmassian , J. Greiner , F. -J. Zickgraf , P. Kroll , J. Krautter , I. Thiering , A. Serrano