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Related papers: Dynamical Modeling of CXOGBS J175553.2-281633: A 1…

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We present phase-resolved spectroscopy and photometry of a source discovered with the Chandra Galactic Bulge Survey (GBS), CXOGBSJ174444.7-260330 (aka CX93 and CX153 in the previously published GBS list). We find two possible values for the…

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 report the discovery of a new catacysmic variable system, RXJ051541+0104.6. The optical spectrum has a blue continuum with superposed H~I and He~I and II emission lines. The soft X-ray spectrum is well fit with a 50~eV black body. The…

Astrophysics · Physics 2009-10-22 F. M. Walter , S. J. Wolk , N. R. Adams

We report optical and infrared observations of the X-ray source CXOGBS J174623.5-310550. This Galactic object was identified as a potential quiescent low-mass X-ray binary accreting from an M-type donor on the basis of optical spectroscopy…

We present X-ray and infrared observations of the X-ray source CXOGC J174536.1-285638. Previous observations suggest that this source may be an accreting binary with a high-mass donor (HMXB) or a colliding wind binary (CWB). Based on the…

We report on ground-based optical observations of ten cataclysmic binaries that were discovered through their X-ray emission. Time-resolved radial velocity spectroscopy yields unambiguous orbital periods for eight objects and ambiguous…

Solar and Stellar Astrophysics · Physics 2015-06-17 John R. Thorstensen , Jules Halpern

We discuss the optical light curves of two Be X-ray Binaries, IGR J06074+2205 and SAX J2103.5+4545 recovered from the ATLAS, ZTF and ASAS-SN databases. Both sources show long term optical variability of 620 and 420 days respectively, with…

High Energy Astrophysical Phenomena · Physics 2024-03-26 Roberto Nesci , Mariateresa Fiocchi , Antonio Vagnozzi

We present the results of a photometric and spectroscopic analysis of the Galactic Bulge Survey X-ray source CXOGBS J174954.5-294335 (hereafter, referred to as CX19). CX19 is a long period, eclipsing intermediate polar type cataclysmic…

Solar and Stellar Astrophysics · Physics 2017-01-17 Christopher B. Johnson , M. A. P. Torres , R. I. Hynes , P. G. Jonker , C. Heinke , T. Maccarone , C. T. Britt , D. Steeghs , T. Wevers , Jianfeng Wu

We report on the discovery of a hydrogen-deficient compact binary (CXOGBS J175107.6-294037) belonging to the AM CVn class in the Galactic Bulge Survey. Deep archival X-ray observations constrain the X-ray positional uncertainty of the…

We conducted time-resolved optical spectroscopy and/or photometry of ten cataclysmic binaries that were discovered in hard X-ray surveys, with the goal of measuring their orbital periods and searching for evidence that they are magnetic.…

High Energy Astrophysical Phenomena · Physics 2022-01-19 J. P. Halpern , J. R. Thorstensen

We present a long-term light curve of the precataclysmic variable (CV) V1082 Sgr obtained by the K2-mission over the course of 81 days. We analyze the entire complex light curve as well as explore several sections in detail with a sliding…

Solar and Stellar Astrophysics · Physics 2018-08-14 Gagik Tovmassian , Paula Szkody , Ricardo Yarza , Mark Kennedy

We present the results of our photometric and spectroscopic studies of the new eclipsing cataclysmic variable star 1RXS J180834.7+101041. Its spectrum exhibits double-peaked hydrogen and helium emission lines. The Doppler maps constructed…

Solar and Stellar Astrophysics · Physics 2015-06-04 D. G. Yakin , V. F. Suleimanov , N. V. Borisov , V. V. Shimanskii , I. F. Bikmaev

We have investigated multiband optical photometric variability and stability of the H$\alpha$ line profile of the transient X-ray binary IGR J01583+6713. We set an upper limit of 0.05 mag on photometric variations in the {\it V} band over a…

Astrophysics · Physics 2009-11-13 Ramanpreet Kaur , Biswajit Paul , Brijesh Kumar , Ram Sagar

In the first paper of this series, we presented a detailed high-resolution spectroscopic study of CPD - 41degr7742, deriving for the first time an orbital solution for both components of the system. In this second paper, we focus on the…

Astrophysics · Physics 2009-09-29 H. Sana , E. Antokhina , P. Royer , J. Manfroid , E. Gosset , G. Rauw , J. -M. Vreux

In course of the search for the optical identifications associated with ROSAT X-ray sources we have found a highly variable object with the very unusual long-term behavior, color indices and high X-ray-to-optical flux ratio. We report the…

Solar and Stellar Astrophysics · Physics 2015-05-28 D. V. Denisenko , A. J. Drake , S. G. Djorgovski , T. V. Kryachko , A. V. Samokhvalov , A. Yu. Tkachenko

We present here results of an optical spectroscopic study of a new Cataclysmic Variable SDSS J001856.93+345444.3. We demonstrate that the most probable value of the orbital period of the system is Porb = 0.6051 \pm 0.022 days (=14.5226…

Solar and Stellar Astrophysics · Physics 2010-09-30 D. Gonzalez , G. Tovmassian , S. Zharikov , A. Aviles , J. Echevarria

We present the first X-ray observations with the XMM-Newton and INTEGRAL satellites of the recently discovered cataclysmic variable 1RXSJ173021.5-055933, together with simultaneous UV and coordinated optical photometry aiming at…

We report on optical imaging of the X-ray binary SAX J1808.4-3658 with the 8-m Gemini South Telescope. The binary, containing an accretion-powered millisecond pulsar, appears to have a large periodic modulation in its quiescent optical…

Astrophysics · Physics 2011-02-11 Zhongxiang Wang , Cees Bassa , Andrew Cumming , Victoria M. Kaspi

1RXS J083842.1$-$282723 is a nearly synchronous magnetic cataclysmic variable with a simple X-ray light curve. While its orbital period was fairly well established at $P_{\rm orb}=98.4$ minutes from optical spectroscopy, indirect estimates…

High Energy Astrophysical Phenomena · Physics 2024-02-02 J. P. Halpern

The gamma-ray binary 1FGL J1018.6-5856 consists of an O6V((f)) type star and an unknown compact object, and shows orbitally modulated emission from radio to very high energy gamma rays. The X-ray light curve shows a maximum around the same…

High Energy Astrophysical Phenomena · Physics 2022-07-06 B. van Soelen , S. Mc Keague , D. Malyshev , M. Chernyakova , N. Komin , N. Matchett , I. M. Monageng
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