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We report on the detection of X-ray pulsations at 2.1 ms from the known X-ray burster IGR J17379-3747 using XMM-Newton. The coherent signal shows a clear Doppler modulation from which we estimate an orbital period of ~1.9 hours and a…

High Energy Astrophysical Phenomena · Physics 2018-09-05 A. Sanna , E. Bozzo , A. Papitto , A. Riggio , C. Ferrigno , T. Di Salvo , R. Iaria , S. M. Mazzola , N. D'Amico , L. Burderi

We report on XMM-Newton and optical results for 6 cataclysmic variables that were selected from Sloan Digital Sky Survey spectra because they showed strong HeII emission lines, indicative of being candidates for containing white dwarfs with…

Solar and Stellar Astrophysics · Physics 2009-11-13 Eric J. Hilton , Paula Szkody , Anjum Mukadam , Arne Henden , William Dillon , Gary D. Schmidt

We report on combined INTEGRAL and XMM-Newton observations of the supergiant fast X-ray transient IGR J16418-4532. The observations targeted the X-ray eclipse region of IGR J16418-4532s orbit with continuous INTEGRAL observations across…

High Energy Astrophysical Phenomena · Physics 2015-06-15 S. P. Drave , A. J. Bird , L. Sidoli , V. Sguera , V. A. McBride , A. B. Hill , A. Bazzano , M. E. Goossens

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

We present the analysis of XMM-Newton European Photon Imaging Camera (EPIC) observations of the nova shell IPHASX J210204.7$+$471015. We detect X-ray emission from the progenitor binary star with properties that resemble those of…

Solar and Stellar Astrophysics · Physics 2021-02-10 J. A. Toalá , G. Rubio , E. Santamaría , M. A. Guerrero , S. Estrada-Dorado , G. Ramos-Larios , L. Sabin

The nature of the X-ray source RX J1914+24 has been the subject of much debate. It shows a prominent period of 569 sec in X-rays and the optical/infra-red: in most models this has been interpreted as the binary orbital period. We present…

Astrophysics · Physics 2009-11-11 Gavin Ramsay , Mark Cropper , Pasi Hakala

In this study, we report a discovery from XMM-Newton, which involves the identification and subsequent examination of a newly discovered polar-type cataclysmic variable named XMM J152737.4-205305.9. The discovery was made by matching the…

High Energy Astrophysical Phenomena · Physics 2024-06-12 Samet Ok , Axel Schwope , David A. H. Buckley , Jaco Brink

We present the results of optical identification of two X-ray sources from RXTE and INTEGRAL all sky surveys: XSS J00564+4548 and IGR J00234+6141. Using the optical data from Russian-Turkish 1.5-m Telescope (RTT150) and SWIFT X-ray…

Astrophysics · Physics 2009-11-11 I. F. Bikmaev , M. G. Revnivtsev , R. A. Burenin , R. A. Sunyaev

We report the discovery of X-ray pulsations at 105.2 Hz (9.5 ms) from the transient X-ray binary IGR J16597-3704 using NuSTAR and Swift. The source was discovered by INTEGRAL in the globular cluster NGC 6256 at a distance of 9.1 kpc. The…

We present analyses of archival X-ray data obtained from the XMM-Newton satellite and optical photometric data obtained from 1 m class telescopes of ARIES, Nainital of a magnetic cataclysmic variable (MCV) Paloma. Two persistent periods at…

Astrophysics of Galaxies · Physics 2016-10-19 Arti Joshi , J. C. Pandey , K. P. Singh , P. C. Agrawal

XMM-Newton observations of the supergiant fast X-ray transient IGR$~$J17544$-$2619 are reported and placed in the context of an analysis of archival INTEGRAL/IBIS data that provides a refined estimate of the orbital period at…

High Energy Astrophysical Phenomena · Physics 2015-06-18 S. P. Drave , A. J. Bird , L. Sidoli , V. Sguera , A. Bazzano , A. B. Hill , M. E. Goossens

IGR J18483-0311 is a poorly known transient hard X-ray source discovered by INTEGRAL during observations of the Galactic Center region performed between 23--28 April 2003. Aims: To detect new outbursts from IGR J18483-0311 using INTEGRAL…

IGR J18483-0311 is a supergiant fast X-ray transient whose compact object is located in a wide (18.5 d) and eccentric (e~0.4) orbit, which shows sporadic outbursts that reach X-ray luminosities of ~1e36 erg/s. We investigated the timing…

High Energy Astrophysical Phenomena · Physics 2015-06-17 L. Ducci , V. Doroshenko , M. Sasaki , A. Santangelo , P. Esposito , P. Romano , S. Vercellone

We report the identification of the cataclysmic variable 1RXSJ062518.2+733433 as an intermediate polar. The orbital period of the system is determined to be 283.0+-2 min from the radial velocity variation of Halpha, measured in an extensive…

Astrophysics · Physics 2009-11-07 S. Araujo-Betancor , B. T. Gaensicke , H. -J. Hagen , P. Rodriguez-Gil , D. Engels

We present data from the first of six monitoring Open Time observations of GRS 1915+105 undertaken with the orbiting INTEGRAL satellite. The source was clearly detected with all three X-ray and gamma-ray instruments on board. GRS 1915+105…

For the past decade, it has been suggested that intermediate polars (IPs), a subclass of magnetic cataclysmic variables (CVs), are one of the main contributors to the hard diffuse X-ray emission from the Galactic center (GC) and Galactic…

High Energy Astrophysical Phenomena · Physics 2022-10-19 Samaresh Mondal , Gabriele Ponti , Frank Haberl , Konstantina Anastasopoulou , Sergio Campana , Kaya Mori , Charles J. Hailey , Nanda Rea

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

IGR J20084+3221 is a previously unclassified Galactic source first detected by INTEGRAL. Chandra observations led to possible classifications of either a magnetic Cataclysmic Variable (mCV) or high mass X-ray binary (HMXB) based on the…

High Energy Astrophysical Phenomena · Physics 2026-05-19 Julian Gerber , Jeremy Hare , John A. Tomsick , Daniel Stern , Aarran W. Shaw

Studying the population of faint hard X-ray sources along the plane of the Galaxy is challenging because of high-extinction and crowding, which make the identification of individual sources more difficult. IGR J18293-1213 is part of the…

High Energy Astrophysical Phenomena · Physics 2016-06-15 Maïca Clavel , J. A. Tomsick , A. Bodaghee , J. -L. Chiu , F. M. Fornasini , J. Hong , R. Krivonos , G. Ponti , F. Rahoui , D. Stern

We report the results of an XMM-Newton and NuSTAR coordinated observation of the Supergiant Fast X-ray Transient (SFXT) IGRJ11215-5952, performed on February 14, 2016, during the expected peak of its brief outburst, which repeats every…

High Energy Astrophysical Phenomena · Physics 2017-04-12 L. Sidoli , A. Tiengo , A. Paizis , V. Sguera , S. Lotti , L. Natalucci