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Related papers: Suzaku observations of the HMXB 1A 1118-61

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We present a timing and broad-band pulse phase resolved spectral analysis of the transient Be X-ray binary pulsar 1A 1118-61 observed during its outburst in January 2009 using Suzaku observations. Suzaku observations were made twice, once…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Chandreyee Maitra , Biswajit Paul , Sachindra Naik

We present the analysis of RXTE monitoring data obtained during the January 2009 outburst of the hard X-ray transient 1A 1118-61. Using these observations the broadband (3.5-120 keV) spectrum of the source was measured for the first time…

High Energy Astrophysical Phenomena · Physics 2015-05-19 V. Doroshenko , S. Suchy , A. Santangelo , R. Staubert , I. Kreykenbohm , R. Rothschild , K. Pottschmidt , J. Wilms

We report the timing and spectral properties of Be/X-ray binary pulsar GX 304-1 by using two Suzaku observations during its 2010 August and 2012 January X-ray outbursts. Pulsations at ~275 s were clearly detected in the light curves from…

Solar and Stellar Astrophysics · Physics 2016-02-16 Gaurava K. Jaisawal , Sachindra Naik , Prahlad Epili

Seventeen accreting neutron star pulsars, mostly high mass X-ray binaries with half of them Be-type transients, are known to exhibit Cyclotron Resonance Scattering Features (CRSFs) in their X-ray spectra, with characteristic line energies…

We present a detailed pulse phase resolved spectral analysis of the persistent high mass X-ray binary pulsar Vela X-1 observed with Suzaku during June 2008. The pulse profiles exhibit both intensity and energy dependence with multiple peaks…

High Energy Astrophysical Phenomena · Physics 2015-06-12 Chandreyee Maitra , Biswajit Paul

The transient X-ray binary pulsar A0535+262 was observed with Suzaku on 2005 September 14 when the source was in the declining phase of the August-September minor outburst. The ~103 s X-ray pulse profile was strongly energy dependent, a…

The accretion-powered pulsar Her X-1 was observed with Suzaku twice in its main-on state, on 2005 October 5-6 and 2006 March 29-30, for a net exposure of 30.5 ks and 34.4 ks, respectively. In the 2005 and 2006 observations, the source was…

We report results of Swift observations for the high mass Be/X-ray binary system 1A 1118-615, during an outburst stage in January, 2009 and at a flaring stage in March, 2009. Using the epoch-folding method, we successfully detected a pulsed…

High Energy Astrophysical Phenomena · Physics 2010-07-19 Lupin Chun-Che Lin , Jumpei Takata , Albert K. H. Kong , Chorng-Yuan Hwang

We present a detailed spectro-temporal study of the Be X-ray binary pulsar $1A$ $1118-61$ during its brightest recorded outburst in 2026, using \textit{Swift} and \textit{NuSTAR} observations, and compare its properties with the 2009…

High Energy Astrophysical Phenomena · Physics 2026-05-19 Kinjal Roy , Aru Beri , Rahul Sharma , Phil Charles

We report the timing and broad-band spectral properties of the Be transient high mass X-ray binary pulsar GRO J1008-57 using a Suzaku observation in the declining phase of its 2007 November-December outburst. Pulsations with a period of…

Solar and Stellar Astrophysics · Physics 2011-05-17 Sachindra Naik , Biswajit Paul , Chetan Kachhara , Santosh V. Vadawale

We analyze the observations of the transient X-ray pulsar 4U 0115+63 with the RXTE and INTEGRAL observatories in a wide X-ray (3-100 keV) energy band during its intense outbursts in 1999 and 2004. The energy of the fundamental harmonic of…

Astrophysics · Physics 2009-06-23 S. S. Tsygankov , A. A. Lutovinov , E. M. Churazov , R. A. Sunyaev

The fastest-rotating magnetar 1E 1547.0-5408 was observed in broad-band X-rays with Suzaku for 33 ks on 2009 January 28-29, 7 days after the onset of its latest bursting activity. After removing burst events, the absorption-uncorrected 2-10…

We report detailed timing and spectral analysis of RXTE-PCA data obtained from observations during the outburst of a transient X-ray pulsar 1A 1118--61 in January 2009. The pulse profile showed significant evolution during the outburst and…

High Energy Astrophysical Phenomena · Physics 2015-05-27 Jincy Devasia , Marykutty James , Biswajit Paul , Kavila Indulekha

We present an analysis of X-ray spectra of the high mass X-ray binary 4U 0115+634 as observed with Suzaku and RXTE in 2011 July, during the fading phase of a giant X-ray outburst. We used a continuum model consisting of an absorbed cutoff…

The 2.1-s anomalous X-ray pulsar 1E 1547.0-5408 exhibited an X-ray outburst on 2009 January 22, emitting a large number of short bursts. The wide-band all- sky monitor (WAM) on-board Suzaku detected at least 254 bursts in the 160keV-6.2MeV…

We present results from two observations of the wind-accreting X-ray pulsar 4U 1907+09 using the Suzaku observatory. The broadband time-averaged spectrum allows us to examine the continuum emission of the source and the cyclotron resonance…

High Energy Astrophysical Phenomena · Physics 2014-11-20 E. Rivers , A. Markowitz , K. Pottschmidt , S. Roth , L. Barragán , F. Fürst , S. Suchy , I. Kreykenbohm , J. Wilms , R. Rothschild

The recurrent hard pulsating X-ray transient \S was observed with \B on March 19, when the source was at a 2--10 keV flux level of $\sim$310~mCrab. We report on the high energy spectrum of the source, concentrating on cyclotron resonant…

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

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…

High Energy Astrophysical Phenomena · Physics 2015-06-16 P. A. Boldin , S. S. Tsygankov , A. A. Lutovinov

We present results obtained from a Suzaku observation of the accretion powered X-ray pulsar GX 1+4. Broad-band continuum spectrum of the pulsar was found to be better described by a simple model consisting of a blackbody component and an…

High Energy Astrophysical Phenomena · Physics 2017-10-17 Yuki Yoshida , Shunji Kitamoto , Hiroo Suzuki , Akio Hoshino , Sachindra Naik , Gaurava K. Jaisawal
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