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Related papers: IPHAS J062746.41+014811.3: a deeply eclipsing inte…

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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…

Detailed timing analyses of three cataclysmic variables, namely 2MASS J09213414$-$5939068, IGR J16167$-$4957, and V667 Pup are carried out using the long-baseline and high-cadence optical photometric data from the Transiting Exoplanet…

Solar and Stellar Astrophysics · Physics 2024-01-30 Arti Joshi

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 on follow-up spectroscopy and photometry of the cataclysmic variable candidate HS0907+1902 selected from the Hamburg Quasar Survey. B, V, and R photometry obtained during the first observed outburst of HS0907+1902 (V~13) reveals…

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

Context: The object HS 0922+1333 was visited briefly in 2002 in a mini survey of low accretion rate polars (LARPs) in order to test if they undergo high luminosity states similar to ordinary polars. On the basis of that short observation…

Astrophysics · Physics 2009-11-13 G. H. Tovmassian , S. V. Zharikov

I conducted photometric observations of the cataclysmic variable LAMOST J035913.61+405035.0 and discovered previously unknown eclipses. During these observations, I recorded 14 eclipses over two groups of nights separated by 13 months. I…

Solar and Stellar Astrophysics · Physics 2024-11-14 V. P. Kozhevnikov

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 on spin variations in the intermediate polar and cataclysmic variable CC Scl, as seen by the Transiting Exoplanet Survey Satellite (TESS). By studying both the spin period and its harmonic, we find that the spin has varied since…

Solar and Stellar Astrophysics · Physics 2024-05-09 John A. Paice , S. Scaringi , N. Castro Segura , A. Sahu , K. Ilkiewicz , Deanne L. Coppejans , D. De Martino , C. Knigge , M. Veresvarska

We report phase-resolved optical polarimetric, photometric and spectroscopic observations of RX J2115.7-5840 (= EUVE J2115-58.6, Craig 1996) which confirms the system to be a magnetic cataclysmic binary of the polar (AM Herculis) subclass.…

Astrophysics · Physics 2009-09-25 A. D. Schwope , D. A. H. Buckley , D. O'Donoghue , G. Hasinger , J. Truemper , W. Voges

We present near-infrared $JHK_s$ photometry and light curves of the candidate magnetic white dwarf+brown dwarf binary SDSS J121209.31+013627.7 and report on the detection of near-infrared excess and variability in the $K_s-$band. The…

Astrophysics · Physics 2009-11-11 J. H. Debes , M. Lopez-Morales , A. Z. Bonanos , A. J. Weinberger

We present optical and X-ray time-series photometry of EI UMa that reveal modulation at 746 and 770 s, which we interpret as the white dwarf spin and spin-orbit sidebands. These detections, combined with previous X-ray studies, establish EI…

Astrophysics · Physics 2009-11-13 Tamara W. Reimer , William F. Welsh , Koji Mukai , F. A. Ringwald

Recent advances in time-domain astronomy have led to fresh observational insights into intermediate polars, a subtype of magnetic cataclysmic variables generally accreting via a partial accretion disc. These new discoveries include…

High Energy Astrophysical Phenomena · Physics 2023-06-07 Koji Mukai , Magaretha L. Pretorius

Optical time series photometry of the short period magnetic white dwarf + probable brown dwarf binary SDSS 121209.31+013627.7 reveals pulse-like variability in all bands from i' to u', peaking at u'. These modulations are most likely due to…

We report the results of a 45 ks Chandra observation of the cataclysmic variable V426 Ophiuchus. The high resolution spectrum from the high-energy transmission grating spectrometer is most consistent with a cooling flow model, placing V426…

We report on high time resolution, high signal/noise, photo-polarimetry of the intermediate polars NY Lup and IGRJ1509-6649. Our observations confirm the detection and colour dependence of circular polarization from NY Lup and additionally…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Stephen B. Potter , Encarni Romero-Colmenero , Marissa Kotze , Ewald Zietsman , O. W. Butters , Nikki Pekeur , David A. H. Buckley

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…

Solar and Stellar Astrophysics · Physics 2016-10-26 J. V. Hernández Santisteban , J. Echevarría , R. Michel , R. Costero

We present the results of photometric CCD observations of the magnetic cataclysmic variable V405 Aurigae (RX J0558.0+5353 = 1RXS J055800.7+535358) obtained using different instruments. We analysed variability of the spin period of the white…

We report the discovery of a relatively bright eclipsing binary system, which consists of a white dwarf and a main sequence K7 star with clear signs of chromospheric and spot activity. The light curve of this system shows $\sim0.2$mag…

Time-resolved CCD photometry is presented of the V~17 optical counterpart of the newly-discovered, hard-X-ray-emitting polar Swift J2619.4+2619. A total of ~20 hr of data obtained over five nights in various bandpasses (B, V, R, and I)…

Astrophysics · Physics 2009-11-13 A. W. Shafter , J. R. A. Davenport , T. Güth , S. Kattner , E. Marin , N. Sreenivasamurthy