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We present new optical spectroscopy of the gamma-ray binary LS 5039. Our data show evidence for sub-orbital modulation in the radial velocities with amplitude ~7 km/s and period ~Porb/4. This short-term oscillation is stable over at least 7…

We present our analysis of new and archived observations of two candidate magnetic cataclysmic variables, namely 1RXS J174320.1-042953 and YY Sex. 1RXS J174320.1-042953 was observed in two distinctive high and low states where a phase shift…

We present a follow-up analysis of the unique magnetic luminosity-variable carbon-atmosphere white dwarf SDSS J142625.71+575218.3. This includes the results of some 106.4 h of integrated light photometry which have revealed, among other…

太阳与恒星天体物理 · 物理学 2009-09-28 E. M. Green , P. Dufour , G. Fontaine , P. Brassard

Hard X-ray light curves and spectral parameters from our analysis of X-ray data of five AM Her type systems - V2301 Oph, V1432 Aql, EP Draconis, GG Leonis, V834 Cen, and one intermediate polar - TV Col, observed using the Rossi X-ray Timing…

天体物理学 · 物理学 2007-05-23 K. P. Singh , V. R. Rana , K. Mukerjee , P. Barrett , E. M. Schlegel

We identify SDSSJ121010.1+334722.9 as an eclipsing post-common-envelope binary, with an orbital period of P ~ 3 hrs, containing a very cool, low-mass, DAZ white dwarf and a low-mass main-sequence star of spectral type M5. A model atmosphere…

The Catalina Real Time Survey (CRTS) has found over 500 cataclysmic variable (CV) candidates, most of which were previously unknown. We report here on followup spectroscopy of 36 of the brighter objects. Nearly all the spectra are typical…

太阳与恒星天体物理 · 物理学 2015-06-05 John R. Thorstensen , Julie N. Skinner

We present a picture of the very unusual blue straggler S1082 in the old open cluster M67 whose light is the sum of a close binary (P = 1.0677978 d) and another cluster member. We provide a complete V-band light curve for the system, and…

天体物理学 · 物理学 2009-11-07 Eric L. Sandquist , David W. Latham , Matthew D. Shetrone , Alejandra A. E. Milone

We report a photometric and spectroscopic study of the peculiar cataclysmic variable SDSS 1507+52. The star shows very deep eclipses on the 67 minute orbital period, and those eclipses are easily separable into white-dwarf and hot-spot…

天体物理学 · 物理学 2009-11-13 J. Patterson , J. R. Thorstensen , C. Knigge

We report on the discovery of J0644+3344, a bright deeply eclipsing cataclysmic variable (CV) binary. Spectral signatures of both binary components and an accretion disk can be seen at optical wavelengths. The optical spectrum shows broad H…

天体物理学 · 物理学 2009-11-13 D. K. Sing , E. M. Green , S. B. Howell , J. B. Holberg , M. Lopez-Morales , J. S. Shaw , G. D. Schmidt

Accurate photometric CoRoT space observations of a secondary seismological target, HD 174884, led to the discovery that this star is an astrophysically important double-lined eclipsing spectroscopic binary in an eccentric orbit (e of about…

太阳与恒星天体物理 · 物理学 2015-05-14 C. Maceroni , J. Montalban , E. Michel , P. Harmanec , A. Prsa , M. Briquet , E. Niemczura , T. Morel , D. Ladjal , M. Auvergne , A. Baglin , F. Baudin , C. Catala , R. Samadi , C. Aerts

2MASS J09440940-5617117 was identified as a cataclysmic variable in 2007 by its spectrum. In this article we present optical differential photometry in the Rc band obtained using the 0.6-m telescope at Observatorio do Pico dos Dias/Brazil.…

太阳与恒星天体物理 · 物理学 2011-02-15 K. M. G. Silva , C. V. Rodrigues , F. J. Jablonski , F. D'Amico , D. Cieslinski , R. Baptista And L. A. De Almeida

New multi-color UBVR light curves of the eclipsing binary KR Cyg were obtained in 2005. Photometric solutions were derived using the Wilson- Devinney method. The result shows that KR Cyg is a near-contact binary system with a large…

太阳与恒星天体物理 · 物理学 2015-06-05 Esin Sipahi

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…

We present spectroscopy of the optical counterpart to 1RXS J162848.1-41524, also known as the microquasar candidate MCQC J162847-4152. All the data indicate that this X-ray source is not a microquasar, and that it is a single-lined…

天体物理学 · 物理学 2009-11-11 M. A. P. Torres , M. R. Garcia , D. Steeghs , J. E. McClintock

We use four years of Kepler photometry to study the non-eclipsing spectroscopic binary KIC 10080943. We find both components to be $\gamma$ Doradus/$\delta$ Scuti hybrids, which pulsate in both p and g modes. We present an analysis of the g…

太阳与恒星天体物理 · 物理学 2015-10-14 M. A. Keen , T. R. Bedding , S. J. Murphy , V. S. Schmid , C. Aerts , A. Tkachenko , R. -M. Ouazzani , D. W. Kurtz

We present B, V, R, I and Z-band photometric observations of HD 209458 during the transit by its planetary companion on UT 1999 November 15 with the University of Hawaii 0.6m and 2.2m telescopes and the High Altitude Observatory STARE…

We report on the discovery of the shortest period binary comprising a hot subdwarf star (CD-30 11223, GALEX J1411-3053) and a massive unseen companion. Photometric data from the All Sky Automated Survey show ellipsoidal variations of the…

太阳与恒星天体物理 · 物理学 2015-06-11 S. Vennes , A. Kawka , S. J. O'Toole , P. Nemeth , D. Burton

We present a CCD photometric study of the star with ASAS ID 134738 + 0410.1 using V band observations obtained from the $IUCAA$ Girawali Observatory (IGO) 2-metre telescope, India. The star was selected from the $\delta$ Scuti database of…

太阳与恒星天体物理 · 物理学 2010-05-24 Sukanta Deb , Harinder P. Singh , T. R. Seshadri , Ranjan Gupta

The majority of magnetic chemically peculiar (mCP) stars exhibit periodic light, magnetic, radio, and spectroscopic variations that can be adequately modelled as a rigidly-rotating main-sequence star with persistent surface structures.…

The Catalina Real-time Transient Survey (CRTS) carried out a public survey for optical transients between 2007 and 2019, discovering more than 16,000 transient candidates. Here we present the spectra and highlight the results of the…

高能天体物理现象 · 物理学 2025-10-27 A. J. Drake , S. G. Djorgovski , M. J. Graham , D. Stern , A. A. Mahabal , M. Catelan , J. L. Prieto , S. Larson