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相关论文: Is FIRST J102347.6+003841 Really a Cataclysmic Bin…

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KIC 9406652 is a cataclysmic variable (CV), sub-classified as `IW And-type star', showing a repetition of standstills with oscillatory variations terminated by brightening. This system showed negative superhumps, semi-periodic variations…

太阳与恒星天体物理 · 物理学 2020-09-30 Mariko Kimura , Yoji Osaki , Taichi Kato

We report the discovery of ZTF J0127+5258, a compact mass-transferring binary with an orbital period of 13.7 minutes. The system contains a white dwarf accretor, which likely originated as a post-common envelope carbon-oxygen (CO) white…

Using a recent Chandra ACIS observation of the eclipsing cataclysmic variable (CV) V1460 Her (2MASS J16211735+4412541) with a fast-rotating ($P_{\rm spin} = 38.9$~s) white dwarf, we estimated a flux $F_{0.5-7 {\rm keV}}^{\rm abs} = (1.9\pm…

太阳与恒星天体物理 · 物理学 2025-01-08 Erik B. Monson , George G. Pavlov , Gordon P. Garmire

We report the discovery of an eclipsing polar, 2XMMi J225036.9+573154, using XMM-Newton. It was discovered by searching the light curves in the 2XMMi catalogue for objects showing X-ray variability. Its X-ray light curve shows a total…

星系天体物理 · 物理学 2009-11-13 Gavin Ramsay , Simon Rosen , Pasi Hakala , Thomas Barclay

We report on the Swift/XRT Deep Galactic Plane Survey discovery and multi-wavelength follow-up observations of a new intermediate polar Cataclysmic Variable, Swift J183920.1-045350. A 449.7 s spin period is found in Xmm-Newton and NuSTAR…

Ground-based long-term optic variability of AM Her, covering the period between 2003-2008, has been conducted to study the features seen in both low and high states of the system. Low-state analysis shows the presence of short-term,…

天体物理学 · 物理学 2009-11-13 Belinda Kalomeni , Kadri Yakut

We present extensive photometric and spectroscopic observations of PTF1 J071912.13+485834.0, an outbursting AM CVn system discovered by the Palomar Transient Factory (PTF). AM CVn systems are stellar binaries with some of the smallest…

Multi-wavelength time-resolved observations of rotationally modulated variability from brown dwarfs and giant exoplanets are the most effective method for constraining their heterogeneous atmospheric structures. In a companion paper (Bowler…

地球与行星天体物理 · 物理学 2022-01-14 Yifan Zhou , Brendan P. Bowler , Caroline V. Morley , Dániel Apai , Tiffany Kataria , Marta L. Bryan , Björn Benneke

Binary radio pulsar system J0737-3039 provides an exceptional opportunity to study innermost structure of pulsar magnetospheres due to very tight orbit, favorable directions of pulsars' rotation and magnetic axes and extremely fortuitous…

天体物理学 · 物理学 2016-08-30 Maxim Lyutikov

PSR J1744-3922 is a binary pulsar exhibiting highly variable pulsed radio emission. We report on a statistical multi-frequency study of the pulsed radio flux variability which suggests that this phenomenon is extrinsic to the pulsar and…

天体物理学 · 物理学 2011-02-11 R. P. Breton , M. S. E. Roberts , S. M. Ransom , V. M. Kaspi , M. Durant , P. Bergeron , A. J. Faulkner

We present the first orbital elements for the massive close binary, HD 101131, one of the brightest objects in the young, open cluster, IC 2944. This system is a double-lined spectroscopic binary in an elliptical orbit with a period of…

天体物理学 · 物理学 2009-11-07 D. R. Gies , L. R. Penny , P. Mayer , H. Drechsel , R. Lorenz

Magnetic cataclysmic variables (CVs) contain a white dwarf with magnetic field strong enough to control the accretion flow from a late type secondary. In this paper, we discover a magnetic CV (CXOGSG J215544.4+380116) from the $Chandra$…

太阳与恒星天体物理 · 物理学 2017-02-01 Song Wang , Yu Bai , Chuan-peng Zhang , Ji-feng Liu

A significant number of cataclysmic variables were detected as hard X-ray sources in the INTEGRAL survey, most of them of the magnetic intermediate polar type. We present a detailed X-ray broad-band study of two new sources, IGR J00234+6141…

太阳与恒星天体物理 · 物理学 2010-07-21 G. Anzolin , D. de Martino , M. Falanga , K. Mukai , J. -M. Bonnet-Bidaud , M. Mouchet , Y. Terada , M. Ishida

We present time-resolved photometry of six faint (V>17mag) cataclysmic variables (CVs); one of them is V849 Oph and the others are identified from the Sloan Digital Sky Survey (SDSS J0920+0042, SDSS J1327+6528, SDSS J1227+5139, SDSS…

太阳与恒星天体物理 · 物理学 2015-05-19 Dicle Zengin Çamurdan , Cafer İbanoğlu , C. Muzaffer Çamurdan

We report the discovery of a new BY Dra-type binary identified as the optical counterpart of the bright source RX J0222.4+4729 detected during the ROSAT All-Sky Survey (Voges et al. 1996). The star is a $V \sim 11.1$, near-by ($\sim 30$…

天体物理学 · 物理学 2009-09-25 Claude Chevalier , Sergio A. Ilovaisky

We used the light curve code XRBinary to model the quiescent K2 light curves of three low-inclination cataclysmic variables (CVs): 1RXS\,J0632+2536 (J0632+2536), RZ\,Leo, TW\,Vir and the pre-CV WD\,1144+011. Optimized light curve models…

We present the discovery of SDSS J135154.46-064309.0, a short-period variable observed using 30-minute cadence photometry in K2 Campaign 6. Follow-up spectroscopy and high-speed photometry support a classification as a new member of the…

We report the discovery of a new cataclysmic variable DDE 32 identified with the ROSAT X-ray source 1RXS J161935.7+524630 in Draco. The variability was originally found by D. Denisenko on the digitized Palomar plates centered at the…

太阳与恒星天体物理 · 物理学 2016-09-28 D. V. Denisenko , F. Martinelli

Near-infrared images of the luminous, high redshift (z=2.1108) radio loud quasar 4C+09.17 reveal a complex structure. The quasar (K=15.76 mag) is surrounded by three "companion" objects having 17.9< K < 20.2 mag at radii of 1.7" < r < 2.9",…

天体物理学 · 物理学 2015-06-24 L. Armus , G. Neugebauer , M. D. Lehnert , K. Matthews

We present high-speed photometry covering one eclipse of the cataclysmic variable system 1RXS J180834.7+101041. The data are modelled as arising from a close binary system containing a low-mass stars filling its Roche lobe plus a white…

太阳与恒星天体物理 · 物理学 2011-01-14 John Southworth , Christopher M Copperwheat