English
Related papers

Related papers: Be X-ray binary pulsar SXP 138: non-linear spin-do…

200 papers

We present the timing and spectral analysis of the HMXB source 4U 1538-522 using NuSTAR observations. One of the observations partially covers the X-ray eclipse of the source along with eclipse ingress. The source is found to spin down at…

High Energy Astrophysical Phenomena · Physics 2023-10-02 Ruchi Tamang , Manoj Ghising , Mohammed Tobrej , Binay Rai , Bikash Chandra Paul

We report on the discovery of X-ray pulsations from the Be/X-ray system LS 992/RX J0812.4-3114 during an RXTE observation. From a timing analysis of the source we obtained a barycentric pulse period of 31.8851 \pm 0.0004 s. The pulse…

Astrophysics · Physics 2009-10-31 Pablo Reig , Paul Roche

We present a detailed timing and spectral analysis of the Be X-ray binary SWJ2000.6+3210 discovered by the BAT Galactic plane survey. Two Suzaku observations of the source made at six months interval, reveal pulsations at ~ 890s for both…

High Energy Astrophysical Phenomena · Physics 2015-06-16 Pragati Pradhan , Chandreyee Maitra , Biswajit Paul , B. C. Paul

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

The Rossi X-ray Timing Explorer has observed five outbursts from the transient 2.5 ms accretion-powered pulsar SAX J1808.4-3658 during 1998-2008. We present a pulse timing study of the most recent outburst and compare it with the previous…

High Energy Astrophysical Phenomena · Physics 2009-09-28 J. M. Hartman , A. Patruno , D. Chakrabarty , C. B. Markwardt , E. H. Morgan , M. van der Klis , R. Wijnands

We report the first hard X-ray (3-79 keV) observations of the millisecond pulsar (MSP) binary PSR J1023+0038 using NuSTAR. This system has been shown transiting between a low-mass X-ray binary (LMXB) state and a rotation-powered MSP state.…

High Energy Astrophysical Phenomena · Physics 2015-06-23 K. L. Li , A. K. H. Kong , J. Takata , K. S. Cheng , P. H. T. Tam , C. Y. Hui , Ruolan Jin

The NuSTAR hard X-ray telescope observed the transient Be/X-ray binary GS 0834-430 during its 2012 outburst - the first active state of this system observed in the past 19 years. We performed timing and spectral analysis, and measured the…

We present RXTE observations of two recently identified massive X-ray binaries. RX J0440.9+4431/BSD 24-491 and RX J1037.5-564/LS 1698 are confirmed as accreting Be/X-ray systems following the discovery of X-ray pulsations, with barycentric…

Astrophysics · Physics 2009-10-31 Pablo Reig , Paul Roche

Recently, there has been renewed interest in the Be X-ray binary (Be/XRB) SAX J1324.4-6200 because of its spatial coincidence with a gamma-ray source detected by Fermi/LAT. To explore more thoroughly its properties, new observations were…

High Energy Astrophysical Phenomena · Physics 2024-05-22 L. Ducci , E. Bozzo , M. Burgay , C. Malacaria , A. Ridolfi , P. Romano , M. M. Serim , S. Vercellone , A. Santangelo

A number of accreting X-ray pulsars experience spectral changes, both on the long time scales and on the time scales of the neutron star spin period. The sources seem to form two distinct groups which differ by the type of the spectral…

High Energy Astrophysical Phenomena · Physics 2015-06-15 Daniela Müller , Dmitry Klochkov , Isabel Caballero , Andrea Santangelo

We report on the XMM-Newton observation of the HMXRB X Persei, the prototype of the persistent and low-luminosity Be/neutron star pulsars, which was performed on February 2003. The source was detected at a luminosity level of ~ 1.4x10^35…

Astrophysics · Physics 2009-11-13 N. La Palombara , S. Mereghetti

In two recent INTEGRAL papers, Lutovinov et al. (2003) and Blay et al. (2004) report a timing and spectral analysis of the transient Be/X-ray pulsar SAX J2103.5+4545 at high energies (5--200 keV). In this work we present for the first time…

We report on the discovery of the new accreting millisecond X-ray pulsar SRGAJ144459.2-604207 using the SRG/ART-XC data. The source was observed twice in February 2024 during the declining phase of the outburst. Timing analysis revealed a…

We report on the first continuous, 80 day optical monitoring of the transitional millisecond pulsar PSR J1023+0038 carried out in mid-2017 with Kepler in the K2 configuration, when an X-ray subluminous accretion disk was present in the…

We present the results obtained from detailed timing and spectral studies of the Be/X-ray binary pulsar KS 1947+300 during its 2013 giant outburst. We used data from Suzaku observations of the pulsar at two epochs i.e. on 2013 October 22…

Solar and Stellar Astrophysics · Physics 2016-05-25 Prahlad Epili , Sachindra Naik , Gaurava K. Jaisawal

We present an X-ray and UV high-time-resolution monitoring of the final flaring phase of the 2022 outburst of the AMSP SAX J1808.4-3658, based on simultaneous XMM-Newton and HST observations. The uninterrupted coverage provided by…

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 present time-resolved optical photometry of the binary millisecond `redback' pulsar PSR J1023+0038 (=AY Sex) during its low-mass X-ray binary phase. The light curves taken between 2014 January and April show an underlying sinusoidal…

High Energy Astrophysical Phenomena · Physics 2015-09-23 T. Shahbaz , M. Linares , S. P. Nevado , P. Rodríguez-Gil , J. Casares , V. S. Dhillon , T. R. Marsh , S. Littlefair , A. Leckngam , S. Poshyachinda

(abridged) We present the results of the long-term hard X-ray monitoring of the high mass X-ray binary 2S 0114+65 with INTEGRAL/IBIS from 2003 to 2008. 2S 0114+65 is a variable hard X-ray source, when 2S 0114+65 was bright, we found a pulse…

High Energy Astrophysical Phenomena · Physics 2015-05-20 Wei Wang

We present results of the first dedicated observation of the young X-ray pulsar SXP 1062 in the broad X-ray energy band obtained during its 2019 outburst with the NuSTAR and XMM-Newton observatories. The analysis of the pulse-phase averaged…

‹ Prev 1 3 4 5 6 7 10 Next ›