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We report the X-ray spectral and timing analysis of the high mass X-ray binary EXO 2030+375 during the 2021 type-II outburst based on the Insight-HXMT observations. Pulsations can be detected in the energy band of 1-150 keV. The pulse…

High Energy Astrophysical Phenomena · Physics 2026-02-11 Yu-Jia Du , Lorenzo Ducci , Long Ji , Qing-Cui Bu , Ling-Da Kong , Peng-Ju Wang , Youli Tuo , Andrea Santangelo

Aims: We investigate the X-ray spectral and timing properties of the high mass X-ray binary EXO 2030+375 observed during its June-September 2006 giant (type II) outburst. Methods: The data analyzed in this work are from partly simultaneous…

The Be X-ray binary EXO 2030+375 went through its third recorded giant outburst from June 2021 to early 2022. We present the results of both spectral and timing analysis based on NICER monitoring, covering the 2-10 keV flux range from 20 to…

We present a type-I outburst of the high-mass X-ray binary EXO 2030+375, detected during INTEGRAL's Performance and Verification Phase in December 2002 (on-source time about 10e+06 seconds). In addition, six more outbursts have been…

In June-September 2006 the Be/X-ray binary EXO 2030+375 experienced the second giant outburst since its discovery. The source was shown to have a complicated pulse-averaged X-ray spectral continuum with possible evidence of cyclotron…

Astrophysics · Physics 2009-11-13 D. Klochkov , A. Santangelo , R. Staubert , C. Ferrigno

In 2021, the high-mass X-ray binary EXO 2030+375 underwent a giant X-ray outburst, the first since 2006, that reached a peak flux of ${\sim}600\,\mathrm{mCrab}$ (3-50\,keV). The goal of this work is to study the spectral evolution over the…

Based on HXMT observations of EXO 2030+375 during its 2021 giant outburst, we report the analysis of pulse variations and the broadband X-ray spectrum, and find the presence of a potential cyclotron resonant scattering feature with the…

High Energy Astrophysical Phenomena · Physics 2024-05-07 Wen Yang , Wei Wang , Prahlad R. Epili

Using BATSE and RXTE observations from 1991 April to 2001 August we have detected 71 outbursts from 82 periastron passages of EXO 2030+375, a 42-second transient X-ray pulsar with a Be star companion, including several outbursts from 1993…

Astrophysics · Physics 2009-11-07 Colleen A. Wilson , Mark H. Finger , M. J. Coe , Silas Laycock , J. Fabregat

In this paper we study the timing and spectral properties of Be/X-ray binary pulsar EXO 2030+375 using a $Suzaku$ observation on 2012 May 23, during a less intense Type I outburst. Pulsations were clearly detected in the X-ray light curves…

Solar and Stellar Astrophysics · Physics 2015-06-23 Sachindra Naik , Gaurava K. Jaisawal

EXO 2030+375 is a peculiar high-mass X-ray binary that has been exhibiting Type-I outburst activities consistently over the past decades. The phases of outburst peaks are generally stable and occur near the orbital periastron.However,…

High Energy Astrophysical Phenomena · Physics 2025-05-09 Run-Ting Huang , Long Ji , Jing-Zhi Yan

We present results from a study of broadband timing and spectral properties of EXO 2030+375 using a Suzaku observation. Pulsations with a period of 41.41 s and strong energy dependent pulse profiles were clearly detected up to ~100 keV.…

High Energy Astrophysical Phenomena · Physics 2013-02-06 Sachindra Naik , Chandreyee Maitra , Gaurava K. Jaisawal , Biswajit Paul

Using the archival RXTE/ASM and SWIFT/BAT observations, the new orbital phases of Type I outbursts of EXO 2030+375 are estimated. A possible correlation between the Type II outburst and optical brightness variations is investigated. In…

Astrophysics · Physics 2009-11-13 A. Baykal , U. Kiziloglu , N. Kiziloglu , E. Beklen , M. Ozbey

We report the evolution of the X-ray pulsations of EXO 2030+375 during its 2021 outburst using the observations from \textit{Insight}-HXMT. Based on the accretion torque model, we study the correlation between the spin frequency derivatives…

In the last 10 years, since its last giant outburst in 2006, regular X-ray outbursts (type I) were detected every periastron passage in the Be X-ray binary EXO 2030+375. Recently, however, it was reported that the source started to show a…

High Energy Astrophysical Phenomena · Physics 2017-01-18 Eva Laplace , Tatehiro Mihara , Yuki Moritani , Motoki Nakajima , Toshihiro Takagi , Kazuo Makishima , Andrea Santangelo

We present a comprehensive timing and spectral studies of Be/X-ray binary pulsar EXO 2030+375 using extensive Rossi X-ray Timing Explorer observations from 1995 till 2011, covering numerous Type I and 2006 Type II outbursts. Pulse profiles…

High Energy Astrophysical Phenomena · Physics 2017-11-08 Prahlad Epili , Sachindra Naik , Gaurava K. Jaisawal , Shivangi Gupta

We study the timing and spectral properties of the X-ray pulsar 2S 1417--624 during the recent outburst in January 2021 based on the Neutron Star Interior Composition Explorer (NICER) observation. We also used some early data from the 2018…

High Energy Astrophysical Phenomena · Physics 2022-11-28 Manoj Mandal , Sabyasachi Pal

The Be X-ray binary pulsar EXO 2030+375, first detected in 1985, has shown a significant detected X-ray outburst at nearly every periastron passage of its 46-day orbit for the past ~25 years, with one low state accompanied by a torque…

During the summer of 2006, the accreting X-ray pulsar EXO 2030+375 underwent its first giant outburst since its discovery in 1985. Our observations include the first ever of the rise of a giant outburst of EXO 2030+375. EXO 2030+375 was…

Astrophysics · Physics 2009-11-13 Colleen A. Wilson , Mark H. Finger , Ascension Camero-Arranz

We present the timing and spectral studies of the Be/X-ray binary XTE J1946+274 during its 2018 and 2021 giant outbursts using observations with the SXT and the LAXPC instruments on the AstroSat satellite. Unlike the 1998 and 2010…

High Energy Astrophysical Phenomena · Physics 2023-02-08 Amar Deo Chandra , Jayashree Roy , P. C. Agrawal

We present a first INTEGRAL observation of the 42s transient X-ray pulsar EXO 2030+375 with IBIS/ISGRI. The source was detected during Cyg X-1 observations in December 2002. We analyzed observations during the outburst period from 9 to 21…

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