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相关论文: X-ray Spectroscopy of the High Mass X-ray Binary P…

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The Be X-ray pulsar SMC X-3 underwent an extra long and ultraluminous giant outburst from 2016 August to 2017 March. The peak X-ray luminosity is up to $\sim 10^{39}$ erg/s, suggesting a mildly super-Eddington accretion onto the strongly…

高能天体物理现象 · 物理学 2018-01-17 Hai-Hui Zhao , Shan-Shan Weng , Ming-Yu Ge , Wei-Hao Bian , Qi-Rong Yuan

XB 1254-690 is a neutron star low-mass X-ray binary with an orbital period of 3.88 hrs, and it exhibits energy-dependent intensity dips, thermonuclear bursts, and flares. We present the results of an analysis of a long observation of this…

High Mass X-ray Binary Pulsars (HMXBP), in which the companion star is a source of supersonic stellar wind, provide a laboratory to probe the velocity and density profile of such winds. Here, we have measured the variation of the absorption…

天体物理学 · 物理学 2009-11-11 U. Mukherjee , B. Paul

We present a broad-band X-ray timing study of the variations in pulse behavior with superorbital cycle in the low-mass X-ray binary Her X-1. This source shows a 35-day superorbital modulation in X-ray flux that is likely caused by…

The Fe K$\alpha$ fluorescence line emission in X-ray spectra is a powerful diagnostic tool for various astrophysical objects to reveal the distribution of cold matter around photo-ionizing sources. The advent of the X-ray microcalorimeter…

We report X-ray observations of the High Mass X-ray Binary (HMXB) pulsar 4U 1907+09. Spectral and Timing analysis of the source has been performed using NuSTAR observation. Timing analysis of the photon events revealed the coherent X-ray…

高能天体物理现象 · 物理学 2022-11-14 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

Cen X-3 shows alternate spin-up/spin-down episodes lasting for tens of days. We study the orbital profiles and spectra of Cen X-3 during these spin-up/spin-down intervals, using long-term data monitored by Fermi/GBM, Swift/BAT and MAXI/GSC.…

高能天体物理现象 · 物理学 2024-01-18 Zhenxuan Liao , Jiren Liu

We report the detection of narrow Fe XXV and Fe XXVI X-ray absorption lines at 6.68 +/- 0.04 keV and 6.97 +/- 0.05 keV in the persistent emission of the dipping low-mass X-ray binary 4U 1323-62 during a 2003 January XMM-Newton observation.…

天体物理学 · 物理学 2009-11-10 L. Boirin , M. Mendez , M. Diaz Trigo , A. N. Parmar , J. S. Kaastra

We report results from long-term (approximately 1240 days) X-ray (0.3-8.0 keV) monitoring of the ultraluminous X-ray source NGC 5408 X-1 with the Swift/X-Ray Telescope. Here we expand on earlier work by Strohmayer (2009) who used only a…

高能天体物理现象 · 物理学 2013-08-09 Dheeraj R. Pasham , Tod E. Strohmayer

We report the discovery of an eclipsing X-ray binary with a 3.62-hr period within 24" of the center of the dwarf starburst galaxy NGC 4214. The orbital period places interesting constraints on the nature of the binary, and allows for a few…

We present broadband X-ray observations of the High Mass X-ray Binary (HMXB) pulsar SMC X-2, using concurrent NuSTAR and NICER observations during its 2022 outburst. The source is found to be spinning with a period of 2.37281(3) s. We…

高能天体物理现象 · 物理学 2025-01-08 Mohammed Tobrej , Binay Rai , Manoj Ghising , Ruchi Tamang , Bikash Chandra Paul

We present results of a comprehensive study of the distribution of absorption dips with orbital phase in Cygnus X-1. Firstly, the distribution was obtained using archival data from all major X-ray observatories and corrected for the…

天体物理学 · 物理学 2009-10-31 M. Balucinska-Church , M. J. Church , P. A. Charles , F. Nagase , J. LaSala , R. Barnard

We present the first results of the observations of the X-ray pulsars LMC X-4, 4U0352+309 and EXO1722-363 performed with the INTEGRAL observatory. The LMC X-4 was investigated during the whole superorbital cycle ($\sim$30 days) and it was…

天体物理学 · 物理学 2007-05-23 A. Lutovinov , S. Tsygankov , M. Revnivtsev , M. Chernyakova , I. Bikmaev , S. Molkov , R. Burenin , N. Sakhibullin

PSR B1259-63 is a 48 ms radio pulsar in a highly eccentric 3.4 year orbit with a Be star SS 2883. Unpulsed gamma-ray, X-ray and radio emission components are observed from the binary system. It is likely that the collision of the pulsar…

星系天体物理 · 物理学 2015-05-13 M. Chernyakova , A. Neronov , F. Aharonian , Y. Uchiyama , T. Takahashi

We report on a long X-ray observation of the slow-rotating binary pulsar GX 1+4. BeppoSAX observed, in the 0.1-200 keV energy range, an event in which the source flux dropped for almost a day, and then recovered. During this event only the…

天体物理学 · 物理学 2015-06-24 Nanda Rea , Luigi Stella , Gian Luca Israel , Giorgio Matt , Silvia Zane , Alberto Segreto , Tim Oosterbroek

We describe the in-orbit performance of the soft X-ray imaging system consisting of the Soft X-ray Telescope and the Soft X-ray Imager aboard Hitomi. Verification and calibration of imaging and spectroscopic performance are carried out…

We present a detailed analysis of observations of the high mass X-ray binary Cen X-3 spanning two consecutive binary orbits performed with the RXTE satellite in early March 1997. The PCA and HEXTE light curves both show a clear reduction in…

We present a timing and spectral analysis of the X-ray pulsar XTE J1946+274 observed with Suzaku during an outburst decline in 2010 October and compare with previous results. XTE J1946+274 is a transient X-ray binary consisting of a Be-type…

We present X-ray observations of the high-inclination low-mass X-ray binary system X2127+119 (AC211) in the globular cluster M15 (NGC 7078). The observations consist of data acquired in 1996 with the RXTE satellite and in 1995 with the ASCA…

天体物理学 · 物理学 2009-11-07 Zach Ioannou , T. Naylor , A. P. Smale , P. A. Charles , K. Mukai

We report NuSTAR observations of the millisecond pulsar - low mass X-ray binary (LMXB) transition system PSR J1023+0038 from June and October 2013, before and after the formation of an accretion disk around the neutron star. Between June…