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Related papers: IGR J18293-1213 is an eclipsing Cataclysmic Variab…

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We present the results of a photometric survey for variable stars in the central region of the nearby globular cluster NGC 6397.Time series photometry was obtained for 30 variable objects. The sample includes 12 new objects, of which 6 show…

Astrophysics · Physics 2009-11-13 J. Kaluzny , I. B. Thompson , W. Krzeminski

IGRJ19294+1816 was discovered by INTEGRAL in 2009 during a bright X-ray outburst and was classified as a possible Be X-ray binary or supergiant fast X-ray transient. On 2010 October 28, the source displayed a second X-ray outburst and a 2…

High Energy Astrophysical Phenomena · Physics 2015-05-28 E. Bozzo , C. Ferrigno , M. Falanga , R. Walter

We report on XMM-Newton, NuSTAR, and NICER X-ray observations of CTCV J2056-3014, a cataclysmic variable (CV) with one of the fastest-spinning white dwarfs (WDs) at P = 29.6 s. While previously classified as an intermediate polar (IP),…

Short time-scale radio variations of compact extragalactic radio quasars and blazars known as IntraDay Variability (IDV) can be explained in at least some sources as a propagation effect; the variations are interpreted as scintillation of…

We report the discovery of SRGE J075818-612027, a deep stream-eclipsing magnetic cataclysmic variable found serendipitously in SRG/eROSITA CalPV observations of the open cluster NGC~2516 as an unrelated X-ray source. An X-ray timing and…

Solar and Stellar Astrophysics · Physics 2023-05-09 Samet Ok , Georg Lamer , Axel Schwope , David A. H. Buckley , Jaco Brink , Jan Kurpas , Dusán Tubín , Iris Traulsen

We use the ROSAT North Ecliptic Pole (NEP) survey to construct a small, but purely X-ray flux-limited sample of cataclysmic variable stars (CVs). The sample includes only 4 systems, 2 of which (RX J1715.6+6856 and RX J1831.7+6511) are new…

Astrophysics · Physics 2009-11-13 M. L. Pretorius , C. Knigge , D. O'Donoghue , J. P. Henry , I. M. Gioia , C. R. Mullis

We study the hard X-ray (20-100 keV) variability of the Galactic Center (GC) and of the nearby sources on the time scale of 1000 s. We find that 3 of the 6 hard X-ray sources detected by INTEGRAL within the central 1 degree of the Galaxy…

Astrophysics · Physics 2007-05-23 A. Neronov , M. Chernyakova , T. J. -L. Courvoisier , R. Walter

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…

The hard X-ray source 2PBC J0658.0-1746 was proposed as an eclipsing magnetic cataclysmic variable of the polar type, based on optical follow-ups. We present the first spectral and timing analysis at X-ray energies with XMM-Newton,…

High Energy Astrophysical Phenomena · Physics 2019-07-24 F. Bernardini , D. de Martino , K. Mukai , M. Falanga , N. Masetti

We report on the spectral and timing properties of the accreting millisecond X-ray pulsar IGR J00291+5934 observed by XMM-Newton and NuSTAR during its 2015 outburst. The source is in a hard state dominated at high energies by a…

High Energy Astrophysical Phenomena · Physics 2017-01-18 A. Sanna , F. Pintore , E. Bozzo , C. Ferrigno , A. Papitto , A. Riggio , T. Di Salvo , R. Iaria , A. D'Aì , E. Egron , L. Burderi

Here, we present the results of our multi-wavelength campaign aimed at classifying \textit{Swift} J170800$-$402551.8 as part of the \textit{Swift} Deep Galactic Plane Survey (DGPS). We utilized Target of Opportunity (ToO) observations with…

Physical parameters of both the mass donor and compact object can be constrained in X-ray binaries with well-defined eclipses, as our survey of wind-fed supergiant X-ray binaries (SGXBs) IGR J16393-4643, IGR J16418-4532, IGR J16479-4514,…

High Energy Astrophysical Phenomena · Physics 2015-08-06 Joel B. Coley , Robin H. D. Corbet , Hans A. Krimm

The short period variable star MG1-688432 has been discovered to exhibit occasional extremely high energy optical outbursts as high as 10^31 joules. Outbursts are typically of several hours duration. These events are often highly…

Solar and Stellar Astrophysics · Physics 2021-08-25 Roy A. Tucker , Eric R. Craine , Brian L. Craine , Andy S. Kulessa , Christopher J. Corbally , Adam L. Kraus

We report on INTEGRAL, Swift and XMM-Newton observations of IGR J17511-3057 performed during the outburst that occurred between March 23 and April 25, 2015. The source reached a peak flux of 0.7(2)E-9 erg/cm$^2$/s and decayed to quiescence…

High Energy Astrophysical Phenomena · Physics 2016-12-07 A. Papitto , E. Bozzo , C. Sanchez-Fernandez , P. Romano , D. F. Torres , C. Ferrigno , J. J. E. Kajava , E. Kuulkers

We report on a broad-band X-ray study (0.5-250 keV) of the Supergiant Fast X-ray Transient IGR J18483-0311 using archival INTEGRAL data and a new targeted XMM-Newton observation. Our INTEGRAL investigation discovered for the first time an…

High Energy Astrophysical Phenomena · Physics 2015-06-23 V. Sguera , L. Sidoli , A. J. Bird , A. Bazzano

The X-ray source IGR J16318-4848 was the first source discovered by INTEGRAL on 2003, January 29. The high energy spectrum exhibits such a high column density that the source is undetectable in X-rays below 2 keV. On 2003, February, 23--25…

Astrophysics · Physics 2007-05-23 Sylvain Chaty , Philippe Filliatre

A growing group of low-mass X-ray binaries are found to be accreting at very-faint X-ray luminosities of <1E36 erg/s (2-10 keV). Once such system is the new X-ray transient IGR J17494-3030. We present Swift and XMM-Newton observations…

High Energy Astrophysical Phenomena · Physics 2015-06-16 M. Armas Padilla , R. Wijnands , N. Degenaar

We present the discovery and multi-wavelength characterization of SRGA J181414.6-225604, a Galactic hard X-ray transient discovered during the ongoing SRG/ART-XC sky survey. Using data from the Palomar Gattini-IR survey, we identify a…

We report the discovery of a new cataclysmic variable MASTER OT J161700.81+620024.9 which is identical to the faint ROSAT X-ray source 1RXS J161659.5+620014. The object was observed in outbursts to 14.4m on 2012 Sep. 11 by MASTER-Tunka and…

Solar and Stellar Astrophysics · Physics 2013-07-30 P. Balanutsa , D. Denisenko , E. Gorbovskoy , V. Lipunov