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We present pulse phase resolved spectra of the hypergiant high mass X-ray binary GX 301-2. We observed the source in 2001 October with RXTE continuously for a total on-source time of almost 200ksec. We model the continuum with both, a…

We present two observations of the high-mass X-ray binary GX 301-2 with NuSTAR, taken at different orbital phases and different luminosities. We find that the continuum is well described by typical phenomenological models, like a very…

高能天体物理现象 · 物理学 2018-12-12 F. Fuerst , S. Falkner , D. Marcu-Cheatham , B. Grefenstette , J. Tomsick , K. Pottschmidt , D. J. Walton , L. Natalucci , P. Kretschmar

We report the orbital X-ray variability of high mass X-ray binary (HMXB) GX301--2. GX301--2 undergone a spin up process in 2018--2020 with the period evolving from $\sim$ 685 s to 670 s. The energy resolved pulse-profiles of the pulsar in…

高能天体物理现象 · 物理学 2022-08-24 Y. Z. Ding , W. Wang , P. R. Epili , Q. Liu , M. Y. Ge , F. J. Lu , J. L. Qu , L. M. Song , S. Zhang , S. N. Zhang

The spectrum of the transient X-ray binary pulsar A0535+26 obtained by OSSE in February 1994 shows an absorption feature at 110 keV but does not confirm a feature at around 55 keV, as previously reported by other instruments. If the 110 keV…

天体物理学 · 物理学 2007-05-23 R. A. Araya , A. K. Harding

We present spectral and timing analysis of NuSTAR observations of RX J0520.5$-$6932 in the 3-79 keV band collected during its outburst in January 2014. The target was observed on two epochs and we report the detection of a cyclotron…

We report the time resolved spectroscopy result from two observations of Cen X-3, over one binary orbit with ASTROSAT and two binary orbit with NuSTAR. NuSTAR covered two intensity states where the light curve showed transition in count…

高能天体物理现象 · 物理学 2023-11-27 Pravat Dangal , Ranjeev Misra , Nand Kumar Chakradhari , Yashpal Bhulla

The present paper reports on the RXTE observations of the binary X-ray pulsar 4U0115+63, covering an outburst in 1999 March-April with 44 pointings. The 3-30 keV PCA spectra and the 15-50 keV HEXTE spectra were analyzed jointly for the…

天体物理学 · 物理学 2008-11-26 Motoki Nakajima , Tatehiro Mihara , Kazuo Makishima , Hisako Niko

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…

高能天体物理现象 · 物理学 2017-05-24 Gaurava K. Jaisawal , Sachindra Naik

We report results of a spectral and timing analysis of the poorly studied transient X-ray pulsar 2S 1553-542 using data collected with the NuSTAR and Chandra observatories and the Fermi/GBM instrument during an outburst in 2015. Properties…

In 2015 October, the Be/X-ray binary 4U 0115+63 underwent a type II outburst, reaching an X-ray luminosity of $\sim$ {\DP{38}\es}. During the outburst, Nuclear Spectroscopic Telescope Array ({\it NuSTAR}) performed two Target of Opportunity…

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

IGR J0607.4+2205 is a transient Be X-ray binary discovered two decades ago. IGR J0607.4+2205 underwent an outburst in 2023 during which it was observed twice with \textit{NuSTAR}. The main goal of this work is to model the broadband X-ray…

高能天体物理现象 · 物理学 2024-02-28 Kinjal Roy , Rahul Sharma , Hemanth Manikantan , Biswajit Paul

We present an in-depth study of the High Mass X-ray Binary (HMXB) GX 301-2 during its pre-periastron flare using data from the XMM-Newton satellite. The energy spectrum shows a power law continuum absorbed by a large equivalent hydrogen…

高能天体物理现象 · 物理学 2011-11-11 F. Fuerst , S. Suchy , I. Kreykenbohm , L. Barragan , J. Wilms , K. Pottschmidt , I. Caballero , P. Kretschmar , C. Ferrigno , R. E. Rothschild

OAO 1657-415 is an accreting X-ray pulsar with a high mass companion that has been observed by several telescopes over the years, in different orbital phases. Back in 1999, observations performed with Beppo-SAX lead to the detection of a…

高能天体物理现象 · 物理学 2022-03-08 Enzo A. Saavedra , Federico A. Fogantini , Jorge A. Combi , Federico García , Sylvain Chaty

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…

An overview of the results of observations for the transient X-ray pulsar 4U 0115+63, a member of a binary system with a Be star, since its discovery to the present day (~40 years) based on data from more than dozen observatories and…

高能天体物理现象 · 物理学 2015-06-16 P. A. Boldin , S. S. Tsygankov , A. A. Lutovinov

In November 2020, A0535+26 underwent one of its brightest outbursts, reaching nearly 12 Crab in X-ray flux. Observed by \textit{Insight-HXMT}, \textit{NuSTAR}, \textit{NICER}, and \textit{AstroSat}, this event provided valuable insights…

高能天体物理现象 · 物理学 2025-01-30 Ashwin Devaraj , Biswajit Paul , Varun Bhalerao , Dipanjan Mukherjee

We report comprehensive spectral and temporal properties of the Be/X-ray binary pulsar SMC X-2 using X-ray observations during the 2015 and 2022 outbursts. The pulse profile of the pulsar is unique and strongly luminosity dependent. It…

高能天体物理现象 · 物理学 2023-03-21 G. K. Jaisawal , G. Vasilopoulos , S. Naik , C. Maitra , C. Malacaria , B. Chhotaray , K. C. Gendreau , S. Guillot , M. Ng , A. Sanna

We present a spectral and timing study of the High Mass X-ray Binary transient source 4U 1700-37 using NuSTAR and ASTROSAT/LAXPC. The source is observed in two different flux states. A combined spectral analysis of NuSTAR's FPMA and FPMB…

高能天体物理现象 · 物理学 2020-03-13 Suman Bala , Jayashree Roy , Dipankar Bhattacharya

We present the results of the neutron star X-ray binary system Cen X-3 performed by $Insight$-HXMT with two observations during 2017 and 2018. During these two observations, the source reached a X-ray luminosity of $\sim 10^{38}$ erg…

高能天体物理现象 · 物理学 2023-05-03 W. Yang , W. Wang , Q. Liu , X. Chen , H. J. Wu , P. F. Tian , J. S. Chen
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