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Related papers: RX J1313.2-3259, a long-period Polar discovered wi…

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We present the study of multi-wavelength observations of an unidentified Fermi Large Area Telescope (LAT) source, 4FGL J1910.7-5320, a new candidate redback millisecond pulsar binary. In the 4FGL 95% error region of 4FGL J1910.7-5320, we…

We have observed the active star $\xi$ Boo A (HD 131156A) with high precision broadband linear polarimetry contemporaneously with circular spectropolarimetry. We find both signals are modulated by the 6.43 day rotation period of $\xi$ Boo…

Magnetars are the most strongly magnetized neutron stars, and one of the most promising targets for X-ray polarimetric measurements. We present here the first Imaging X-ray Polarimetry Explorer (IXPE) observation of the magnetar 1RXS…

High Energy Astrophysical Phenomena · Physics 2023-02-22 Silvia Zane , Roberto Taverna , Denis Gonzalez Caniulef , Fabio Muleri , Roberto Turolla , Jeremy Heyl , Keisuke Uchiyama , Mason Ng , Toru Tamagawa , Ilaria Caiazzo , Niccolo' Di Lalla , Herman L. Marshall , Matteo Bachetti , Fabio La Monaca , Ephraim Gau , Alessandro Di Marco , Luca Baldini , Michela Negro , Nicola Omodei , John Rankin , Giorgio Matt , George G. Pavlov , Takao Kitaguchi , Henric Krawczynski , Fabian Kislat , Ruth Kelly , Ivan Agudo , Lucio A. Antonelli , Wayne H. Baumgartner , Ronaldo Bellazzini , Stefano Bianchi , Stephen D. Bongiorno , Raffaella Bonino , Alessandro Brez , Niccolo' Bucciantini , Fiamma Capitanio , Simone Castellano , Elisabetta Cavazzuti , Chieng Ting Chen , Stefano Ciprini , Enrico Costa , Alessandra De Rosa , Ettore Del Monte , Laura Di Gesu , Immacolata Donnarumma , Victor Doroshenko , Michal Dovciak , Steven R. Ehlert , Teruaki Enoto , Yuri Evangelista , Sergio Fabiani , Riccardo Ferrazzoli , Javier A. Garcia , Shuichi Gunji , Kiyoshi Hayashida , Wataru Iwakiri , Svetlana G. Jorstad , Philip Kaaret , Vladimir Karas , Jeffery J. Kolodziejczak , Luca Latronico , Ioannis Liodakis , Simone Maldera , Alberto Manfreda , Frederic Marin , Andrea Marinucci , Alan P. Marscher , Francesco Massaro , Ikuyuki Mitsuishi , Tsunefumi Mizuno , C. Y. Ng , Stephen L. O'Dell , Chiara Oppedisano , Alessandro Papitto , Abel L. Peirson , Matteo Perri , Melissa Pesce Rollins , Pierre Olivier Petrucci , Maura Pilia , Andrea Possenti , Juri Poutanen , Simonetta Puccetti , Brian D. Ramsey , Ajay Ratheesh , Oliver J. Roberts , Roger W. Romani , Carmelo Sgro' , Patrick Slane , Paolo Soffitta , Gloria Spandre , Douglas A. Swartz , Fabrizio Tavecchio , Yuzuru Tawara , Allyn F. Tennant , Nicholas E. Thomas , Francesco Tombesi , Alessio Trois , Sergey S. Tsygankov , Jacco Vink , Martin C. Weisskopf , Kinwah Wu , Fei Xie

The high-mass X-ray binary RX J0146.9+6121, with optical counterpart LS I+61 235 (V831 Cas), is an intriguing system on the outskirts of the open cluster NGC 663. It contains the slowest X-ray pulsar known with a pulse period of around…

Until now X-radiation from nine millisecond pulsars has been detected. In the present paper we summarize the observations and show the results of a re-analysis of archival ROSAT data. In addition we present the results of recent…

Astrophysics · Physics 2007-05-23 W. Becker , J. Trümper

We present an analysis of X-ray, Ultraviolet and optical/near-IR photometric data of the transitional millisecond pulsar binary XSSJ12270-4859, obtained at different epochs after the transition to a rotation-powered radio pulsar state. The…

Using X-ray data from the Rossi X-Ray Timing Explorer (RXTE), we carried out pulse timing analysis of the transient X-ray pulsar SAX J2103.5+4545. An outburst was detected by All Sky Monitor (ASM) October 25 1999 and reached a peak X-ray…

Astrophysics · Physics 2009-10-31 A. Baykal , M. Stark , J. Swank

High-resolution spectroscopy and photometric monitoring of the pre-main sequence star RXJ1608.6-3922 shows that it is not an eclipsing binary, as previously claimed. Radial velocity measurements covering suitable time spans in order to…

Astrophysics · Physics 2009-11-06 V. Joergens , E. Guenther , R. Neuhäuser , M. Fernández , J. Vijapurkar

We report on observations of the sixth accretion-powered millisecond pulsar, IGR J00291+5934, with the Rossi X-Ray Timing Explorer. The source is a faint, recurrent X-ray transient initially identified by INTEGRAL. The 599 Hz (1.67 ms)…

Astrophysics · Physics 2009-11-10 D. K. Galloway , C. B. Markwardt , E. H. Morgan , D. Chakrabarty , T. E. Strohmayer

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…

RX J0513.1+0851 and RX J0539.9+0956 were previously identified as young, low-mass, single-lined spectroscopic binary systems and classified as weak-lined T Tauri stars at visible wavelengths. Here we present radial velocities, spectral…

Solar and Stellar Astrophysics · Physics 2015-06-15 Dary Ruíz-Rodríguez , L. Prato , Guillermo Torres , L. H. Wasserman , Ralph Neuhäuser

We report the detection of modulated circular polarization in V795 Her. The degree of polarization increases with wavelength and is modulated with a period of 19.54 min, which is very close to the reported optical QPO period. The modulation…

Astrophysics · Physics 2007-05-23 P. Rodriguez-Gil , J. Casares , I. G. Martinez-Pais , P. Hakala

The radio and gamma-ray pulsar PSR J2032+4127 was recently found to be in a decades-long orbit with the Be star MT91 213, with the pulsar moving rapidly towards periastron. This binary shares many similar characteristics with the previously…

Solar and Stellar Astrophysics · Physics 2016-10-26 Wynn C. G. Ho , C. -Y. Ng , Andrew G. Lyne , Ben W. Stappers , Malcolm J. Coe , Jules P. Halpern , Tyrel J. Johnson , Iain A. Steele

We report the results of an analysis of data obtained with the INTEGRAL, Swift and RXTE observatories during the 2010 April and September outbursts of the X-ray pulsar RX J0440.9+4431. The temporal and spectral properties of the pulsar in a…

High Energy Astrophysical Phenomena · Physics 2015-06-03 S. Tsygankov , R. Krivonos , A. Lutovinov

We report the discovery of an eclipsing X-ray binary in M101, the first such system to be discovered outside the Local Group. Based on a sequence of 25 Chandra observations that sample a wide range of orbital phases, we find a period of…

Astrophysics · Physics 2008-11-26 Jifeng Liu , Rosanne di Stefano , Jeffrey McClintock , Albert Kong , Joel Bregman , Kip Kuntz

We report pulsations in the X-ray flux of RX J0101.3-7211 in the Small Magellanic Cloud (SMC) with a period of 455+/-2 s in XMM-Newton EPIC-PN data. The X-ray spectrum can be described by a power-law with a photon index of 0.6+/-0.1. Timing…

Astrophysics · Physics 2009-11-06 M. Sasaki , F. Haberl , S. Keller , W. Pietsch

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…

Astrophysics · Physics 2007-05-23 K. P. Singh , V. R. Rana , K. Mukerjee , P. Barrett , E. M. Schlegel

Using the Mikhail Pavlinsky ART-XC onboard the SRG observatory we have detected, for the first time, X-ray pulsations with a period of ~106 s from the poorly-studied high-mass X-ray binary RX J0535.0-6700 located in the Large Magellanic…

High Energy Astrophysical Phenomena · Physics 2025-05-09 I. A. Mereminskiy , A. S. Gorban , Yu. S. Klein , E. A. Ushakova , A. N. Semena , A. A. Lutovinov , A. Yu. Tkachenko , S. V. Molkov

We report the discovery of a highly X-ray variable AGN, RX J2217.9-5941. This object was bright during the ROSAT All-Sky Survey (RASS), during which a decrease in the count rate by a factor of 12 was observed. It was found to be much…

Astrophysics · Physics 2009-11-06 D. Grupe , H. -C. Thomas , K. M. Leighly

We present a combined analysis of XMM-Newton, Chandra and Rosat observations of the isolated neutron star RXJ0720.4-3125, spanning a total period of \sim 7 years. We develop a maximum likelihood periodogramme for our analysis based on the…

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