中文
相关论文

相关论文: Nustar observation of the binary system 4U 0114+65

200 篇论文

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

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…

天体物理学 · 物理学 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;…

高能天体物理现象 · 物理学 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…

天体物理学 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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,…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 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…

高能天体物理现象 · 物理学 2017-12-27 Aditya S. Mondal , Gulab C. Dewangan , Mayukh Pahari , Biplab Raychaudhuri