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Related papers: Variable Absorption Line in XTE J1810-197

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Because of its complex clumpy wind, prominent cyclotron resonant scattering features, intrinsic variability and convenient physical parameters (close distance, high inclination, small orbital separation) which facilitate the observation and…

High Energy Astrophysical Phenomena · Physics 2022-04-20 C. M. Diez , V. Grinberg , F. Fürst , E. Sokolova-Lapa , A. Santangelo , J. Wilms , K. Pottschmidt , S. Martínez-Núñez , C. Malacaria , P. Kretschmar

We have investigated the radio emission from the anomalous X-ray pulsar 1E 1547.0-5408 (PSR J1550-5418) using the Parkes telescope and the Australia Telescope Compact Array. The flux density of the pulsar is roughly the same between 1.4 and…

Astrophysics · Physics 2009-11-13 F. Camilo , J. Reynolds , S. Johnston , J. P. Halpern , S. M. Ransom

We report broadband spectral properties of the high mass X-ray binary pulsar SMC X-2 by using three simultaneous $NuSTAR$ and $Swift$/XRT observations during its 2015 outburst. The pulsar was significantly bright, reaching a luminosity up…

High Energy Astrophysical Phenomena · Physics 2017-05-24 Gaurava K. Jaisawal , Sachindra Naik

We report on the results of a detailed phase-resolved spectroscopy of archival XMM--Newton observations of X-ray Dim Isolated Neutron Stars (XDINSs). Our analysis revealed a narrow and phase-variable absorption feature in the X-ray spectrum…

High Energy Astrophysical Phenomena · Physics 2017-05-03 A. Borghese , N. Rea , F. Coti Zelati , A. Tiengo , R. Turolla , S. Zane

We present the results of the pulse phase- and luminosity-resolved spectroscopy of the transient X-ray pulsar V0332+53, performed for the first time in a wide luminosity range (1-40)x10^{37} erg/s during a giant outburst observed by the…

High Energy Astrophysical Phenomena · Physics 2015-06-23 A. A. Lutovinov , S. S. Tsygankov , V. F. Suleimanov , A. A. Mushtukov , V. Doroshenko , D. I. Nagirner , J. Poutanen

We report results of the INTEGRAL Target of Opportunity observations of the transient X-ray burster XTE J1810-189. The observations were performed on April 3--6, 2008, soon after the discovery of the source and near the peak of its…

High Energy Astrophysical Phenomena · Physics 2010-04-26 I. Chelovekov , S. Grebenev

The transient X-ray source MAXI J1810-222 was discovered in 2018 and has been active ever since. A long combined radio and X-ray monitoring campaign was performed with ATCA and Swift respectively. It has been proposed that MAXI J1810-222 is…

High Energy Astrophysical Phenomena · Physics 2023-05-03 M. Del Santo , C. Pinto , A. Marino , A. D'Aì , P. -O. Petrucci , J. Malzac , J. Ferreira , F. Pintore , S. E. Motta , T. D. Russell , A. Segreto , A. Sanna

We report on the discovery of a transient X-ray pulsar, AX J1841.0-0536, serendipitously found in the Scutum arm region with the ASCA in two separate observations. The X-ray flux is very faint at the beginning, but exhibits two flares in…

Astrophysics · Physics 2015-06-24 Aya Bamba , Jun Yokogawa , Masaru Ueno , Katsuji Koyama , Shigeo Yamauchi

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

The existence of radio pulsars having inferred magnetic fields in the magnetar regime suggests that possible transition objects could be found in the radio pulsar population. The discovery of such an object would contribute greatly to our…

Astrophysics · Physics 2008-11-26 M. E. Gonzalez , V. M. Kaspi , F. Camilo , B. M. Gaensler , M. J. Pivovaroff

The accreting millisecond pulsar XTE J1814-338 exhibits oscillations at the known spin frequency during Type I X-ray bursts. The properties of the burst oscillations reflect the nature of the thermal asymmetry on the stellar surface. We…

Astrophysics · Physics 2009-11-13 Anna L. Watts , Tod E. Strohmayer , Craig B. Markwardt

The variable X-ray source 1E 1547.0-5408 was identified by Gelfand & Gaensler (2007) as a likely magnetar in G327.24-0.13, an apparent supernova remnant. No X-ray pulsations have been detected from it. Using the Parkes radio telescope, we…

Astrophysics · Physics 2009-11-13 F. Camilo , S. M. Ransom , J. P. Halpern , J. Reynolds

We report on X-ray monitoring of two isolated pulsars within the same RXTE field of view. PSR J1811-1925 in the young supernova remnant G11.2-0.3 has a nearly sinusoidal pulse profile with a hard pulsed spectrum (photon index \~1.2). The…

Multiwavelength observations have revealed the highly unusual properties of the gamma-ray source PMN J1603-4904, which are difficult to reconcile with any other well established gamma-ray source class. The object is either a very atypical…

We report evidence for an ~ 80 d periodicity in the X-ray flux of the hard transient pulsar XTE J1946+274. The 1.3-12 keV light curve obtained with the RossiXTE All Sky Monitor shows five regularly spaced flares over a ~ 1 year baseline…

Astrophysics · Physics 2007-05-23 Sergio Campana , Gianluca Israel , Luigi Stella

We report the accurate sub-arcsec X-ray position of the new Anomalous X-ray Pulsar (AXP) XTE J1810-197, derived with a Chndra-HRC Target of Opportunity observation carried out in November 2003. We also report the discovery of a likely IR…

We have analyzed the new deep {\it XMM-Newton} and {\it Chandra} observations of the energetic radio-quiet pulsar J1813$-$1246. The X-ray spectrum is non-thermal, very hard and absorbed. Based on spectral considerations, we propose that…

High Energy Astrophysical Phenomena · Physics 2015-06-22 M. Marelli , A. Harding , D. Pizzocaro , A. De Luca , K. S. Wood , P. Caraveo , D. Salvetti , P. M. Saz Parkinson , F. Acero

We report on a detailed spectral analysis of emission from X-ray pulsar 4U 1901+03 using data obtained by the Insight-HXMT and NuSTAR observatories during the 2019 outburst of the source. Thanks to the extensive coverage of the outburst by…

We report the results of new XMM-Newton observations of the middle-aged ($\sim$10$^5$ yr) radio pulsar PSR J1740+1000 carried out in 2017-2018. These long pointings ($\sim$530 ks) show that the non-thermal emission, well described by a…

High Energy Astrophysical Phenomena · Physics 2022-05-04 Michela Rigoselli , Sandro Mereghetti , Sara Anzuinelli , Michael Keith , Roberto Taverna , Roberto Turolla , Silvia Zane

We analyze the emission and absorption lines during photospheric radius expansion (PRE) X-ray bursts from the ultracompact binary 4U 1820--30, observed with the Neutron Star Interior Composition Explorer (NICER). Using Monte Carlo…

High Energy Astrophysical Phenomena · Physics 2025-04-16 Wenhui Yu , Zhaosheng Li , Yuanyue Pan , Xuejuan Yang , Yupeng Chen , Shu Zhang , Maurizio Falanga
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