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Related papers: The peculiar high-mass X-ray binary 1ES 1210-646

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The source IGR J17200-3116 was discovered in the hard X-ray band by INTEGRAL. A periodic X-ray modulation at ~326 s was detected in its Swift light curves by our group (and subsequently confirmed by a Swift campaign). In this paper, we…

High Energy Astrophysical Phenomena · Physics 2014-06-06 P. Esposito , G. L. Israel , L. Sidoli , A. Tiengo , S. Campana , A. Moretti

The origin of the multiwavelength emission from the high-synchrotron-peaked BL Lac 1ES 1218+304 is studied using the data from {\it Swift UVOT/XRT}, {\it NuSTAR} and {\it Fermi-LAT}. A detailed temporal and spectral analysis of the data…

High Energy Astrophysical Phenomena · Physics 2020-07-08 N. Sahakyan

We report the detection of orbital modulation, a model solution, and X-ray properties of a newly discovered contact binary, 2MASS J11201034$-$2201340. We serendipitously found this X-ray point source outside the error ellipse when searching…

We report on the first spectral and timing characterization of the transient X-ray source 1RXS J194211.9+255552 using all available data from the Swift X-ray satellite. We used 10 years of hard X-ray data from the Burst Alert Telescope…

High Energy Astrophysical Phenomena · Physics 2016-01-14 A. D'Aì , G. Cusumano , V. La Parola , A. Segreto

Low-mass X-ray binaries are binary systems composed of a compact object and a low-mass star. Recently, a new class of these systems, known as symbiotic $X$-ray binaries (with a neutron star with a M-type giant companion), has been…

Astrophysics · Physics 2009-11-13 A. A. Nucita , S. Carpano , M. Guainazzi

We analyze 1050 ks of INTEGRAL data of the high mass X-ray binary pulsar 1E 1145.1-6141 to study its properties over a long time baseline, from June 2003 to June 2004, with wide spectral coverage. We study three high luminosity episodes,…

(abridged) We present the results of the long-term hard X-ray monitoring of the high mass X-ray binary 2S 0114+65 with INTEGRAL/IBIS from 2003 to 2008. 2S 0114+65 is a variable hard X-ray source, when 2S 0114+65 was bright, we found a pulse…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Wei Wang

We present a comprehensive multi-frequency study of the HBL 1ES 1959+650 using data from various facilities during the period 2016-2017, including X-ray data from {\it AstroSat} and {\it Swift} during the historically high X-ray flux state…

U 2206+54 is a wind-fed high mass X-ray binary with a main-sequence donor star. The nature of its compact object was recently identified as a slow-pulsation magnetized neutron star. INTEGRAL/IBIS observations have a long-term hard X-ray…

High Energy Astrophysical Phenomena · Physics 2015-05-19 W. Wang

XSS J12270-4859 (J12270) is an enigmatic source of unknown nature. Previous studies revealed that the source has unusual X-ray temporal characteristics, including repetitive short-term flares followed by spectral hardening, non-periodic…

High Energy Astrophysical Phenomena · Physics 2015-05-28 Kei Saitou , Masahiro Tsujimoto , Ken Ebisawa , Manabu Ishida , Koji Mukai , Takahiro Nagayama , Shogo Nishiyama , Poshak Gandhi

Understanding how black holes accrete and supply feedback to their environment is one of the outstanding challenges of modern astrophysics. Swift J1910.2-0546 is a candidate black hole low-mass X-ray binary that was discovered in 2012 when…

We present the results of a detailed study of the high mass X-ray binary 2S 0114+650 made with the pointed instruments onboard the Rossi X-ray Timing Explorer. The spectral and temporal behaviour of this source was examined over the pulse,…

Astrophysics · Physics 2010-01-04 S. A. Farrell , R. K. Sood , P. M. O'Neill , S. Dieters

We have observed the eclipsing low-mass X-ray binary MS1603.6+2600 with Chandra for 7 ksec. The X-ray spectrum is well fit with a single absorbed powerlaw with an index of ~2. We find a clear sinusoidal modulation in the X-ray lightcurve…

Astrophysics · Physics 2009-11-10 P. G. Jonker , M. van der Klis , C. Kouveliotou , M. Mendez , W. H. G. Lewin , T. Belloni

The nature of the hard X-ray source XSSJ12270-4859 is still unclear though it was claimed to be a magnetic Cataclysmic Variable. We here present a broad-band X-ray and gamma ray study based on a recent XMM-Newton observation and archival…

High Energy Astrophysical Phenomena · Physics 2015-05-18 D. de Martino , M. Falanga , J. -M. Bonnet-Bidaud , T. Belloni , M. Mouchet , N. Masetti , I. Andruchow , S. A. Cellone , K. Mukai , G. Matt

We report the identification of the ROSAT all-sky survey source 1RXS J154814.5-452845as new intermediate polar and present the results from follow-up optical and X-ray observations. The source shows pulsations with a period of 693 s both in…

Astrophysics · Physics 2009-11-07 F. Haberl , C. Motch , F. -J. Zickgraf

The bright eclipsing and bursting low-mass X-ray binary EXO 0748-676 has been observed at several occasions by XMM-Newton during the initial calibration and performance verification (CAL/PV) phase. We present here the results obtained from…

Astrophysics · Physics 2009-10-31 J. M. Bonnet-Bidaud , F. Haberl , P. Ferrando , P. J. Bennie , E. Kendziorra

(Abridged) Spectral and time variability analysis of the region of the hard X-ray transient EXS 1737.9-2952 near the Galactic Centre (GC), using data from the Narrow Field Instruments of BeppoSAX is reported. The main results are the MECS…

Astrophysics · Physics 2007-05-23 J. Huovelin , J. Schultz , O. Vilhu , D. Hannikainen , P. Muhli , Ph. Durouchoux

LSI +61 303 is one of the most interesting high-mass X-ray binaries owing to its spatially resolved radio emission and its TeV emission, generally attributed to non-thermal particles in an accretion-powered relativistic jet or in the…

Astrophysics · Physics 2009-02-23 P. Esposito , P. A. Caraveo , A. Pellizzoni , A. De Luca , N. Gehrels , M. A. Marelli

We report results of the first detailed spectral and temporal studies of the recently discovered Be/X-ray binary eRASSU J050810.4$-$660653 in LMC based on the data from the SRG/ART-XC, NuSTAR and Swift/XRT instruments obtained in December…

X-ray observations are essential to achieve a deeper understanding of the broadband emission mechanism in blazars. Here, we present a long-term spectral and temporal analysis of X-ray and optical observations of 1E 0229+200 collected with…

High Energy Astrophysical Phenomena · Physics 2025-10-20 Alicja Wierzcholska , Hubert Siejkowski
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