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Related papers: Nustar observation of the binary system 4U 0114+65

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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 the results of a series of XMM-Newton EPIC and OM observations of Her X-1, spread over a wide range of the 35 d precession period. We confirm that the spin modulation of the neutron star is weak or absent in the low state - in…

Astrophysics · Physics 2009-11-10 S. Zane , G. Ramsay , M. A. Jimenez-Garate , J. W. den Herder , M. Still , P. T. Boyd , C. J. Hailey

Symbiotic X-ray binaries form a subclass of low-mass X-ray binary systems consisting of a neutron star accreting material from a red giant donor star via stellar wind or Roche lobe overflow. Only a few confirmed members are currently known;…

High Energy Astrophysical Phenomena · Physics 2015-06-18 A. A. Nucita , S. Stefanelli , F. De Paolis , N. Masetti , G. Ingrosso , M. Del Santo , L. Manni

Unique among neutron stars, 1E 1207.4-5209 is an X-ray pulsar with a spin period of 424 ms that contains at least two strong absorption features in its energy spectrum. This neutron star has been identified as a member of the radio-quiet…

Astrophysics · Physics 2008-11-26 Peter M. Woods , Vyacheslav E. Zavlin , George G. Pavlov

We report results of the first detailed spectral and temporal studies of the recently discovered Be/X-ray binary eRASSU J050810.4$-$660653 in LMC based on the data from the SRG/ART-XC, NuSTAR and Swift/XRT instruments obtained in December…

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…

The low mass X-ray binary 4U 2129+47 was discovered during a previous X-ray outburst phase and was classified as an accretion disk corona source. A 1% delay between two mid-eclipse epochs measured ~22 days apart was reported from two…

High Energy Astrophysical Phenomena · Physics 2014-11-20 Jinrong Lin , Michael A. Nowak , Deepto Chakrabarty

We report the results from a detailed timing and spectral study of transient X-ray pulsars, 4U 1901+03 during its 2019 outburst. We performed broadband spectroscopy in the 1-70 keV energy band using four observations made with Swift and…

High Energy Astrophysical Phenomena · Physics 2020-11-04 Aru Beri , Tinku , Nirmal K. Iyer , Chandreyee Maitra

We report on the first NuSTAR observation of the transitional millisecond pulsar binary XSS J12270-4859 during its current rotation-powered state, complemented with a 2.5yr-long radio monitoring at Parkes telescope and archival XMM-Newton…

High Energy Astrophysical Phenomena · Physics 2020-01-24 D. de Martino , A. Papitto , M. Burgay , A. Possenti , F. Coti Zelati , N. Rea , D. F. Torres , T. M. Belloni

In this study, we examine 51 archival NICER observations and 6 archival NuSTAR observations of the neutron star (NS) ultra-compact X-ray binary (UCXB) 4U 0614+091, which span over 5 years. The source displays persistent reflection features,…

High Energy Astrophysical Phenomena · Physics 2024-09-17 David L. Moutard , Renee M. Ludlam , Edward M. Cackett , Javier A. García , Jon M. Miller , Dan R. Wilkins

We have studied the timing and spectral properties of the BeXB 4U 1901+03 during the 2019 outburst using \textit{NuSTAR}, \textit{Swift}, and \textit{NICER} observations. Flares are in all observations and were of tens to hundreds of…

High Energy Astrophysical Phenomena · Physics 2021-09-08 Binay Rai , Bikash Chandra Paul

Burst oscillations during thermonuclear X-ray bursts are powered by thermonuclear energy on the neutron star (NS) surface and typically occur close to the spin frequency of the NS. We performed a comprehensive timing analysis of all…

High Energy Astrophysical Phenomena · Physics 2026-03-16 Manoj Mandal , Sachindra Naik

We report on the results of a NuSTAR observation of the Supergiant Fast X-ray Transient pulsar IGRJ11215-5952 during the peak of its outburst in June 2017. IGRJ11215-5952 is the only SFXT undergoing strictly periodic outbursts, every 165…

High Energy Astrophysical Phenomena · Physics 2020-07-01 L. Sidoli , K. Postnov , A. Tiengo , P. Esposito , V. Sguera , A. Paizis , G. A. Rodrıguez Castillo

We present here the results of broadband spectral analysis of low-mass X-ray binary and a black hole candidate 4U 1957+11. The source was observed nine times with the Nuclear Spectroscopic Telescope Array (NuSTAR) between 2018 September and…

High Energy Astrophysical Phenomena · Physics 2021-11-24 Prince Sharma , Rahul Sharma , Chetana Jain , Gulab C. Dewangan , Anjan Dutta

We report the quasi-simultaneous INTEGRAL, SWIFT, and NuSTAR observations showing spectral state transitions in the neutron star low mass X-ray binary 1RXS J180408.9-342058 during its 2015 outburst. We present results of the analysis of…

High Energy Astrophysical Phenomena · Physics 2020-01-08 M. Fiocchi , A. Bazzano , G. Bruni , R. Ludlam , L. Natalucci , F. Onori , P. Ubertini

JWST observed the magnetar 4U 0142+61 with the MIRI and NIRCam instruments within a 77 min time interval on 2022 September 20-21. The low-resolution MIRI spectrum and NIRCam photometry show that the spectrum in the wavelength range 1.4-11…

High Energy Astrophysical Phenomena · Physics 2024-07-19 Jeremy Hare , George G. Pavlov , Bettina Posselt , Oleg Kargaltsev , Tea Temim , Steven Chen

We present observations of the historic transient 4U 1730-22 as observed with the Neutron Star Interior Composition Explorer (NICER). After remaining in quiescence since its 1972 discovery, this X-ray binary showed renewed outburst activity…

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

We report a NuSTAR observation of a solar microflare, SOL2015-09-01T04. Although it was too faint to be observed by the GOES X-ray Sensor, we estimate the event to be an A0.1 class flare in brightness. This microflare, with only 5 counts…

We report on the \nustar{} observation of the Z-type neutron star low-mass X-ray binary Cygnus X--2 performed on 7 January 2015. During this observation, the source exhibited sudden decrease in count rate (dips) and stronger variability in…

High Energy Astrophysical Phenomena · Physics 2017-12-27 Aditya S. Mondal , Gulab C. Dewangan , Mayukh Pahari , Biplab Raychaudhuri
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