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相关论文: The thermonuclear X-ray bursts of 4U 1730-22

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A type-I burst could influence the accretion process through radiation pressure and Comptonization both for the accretion disk and the corona/boundary layer of an X-ray binary, and vice versa. We investigate the temporal evolution of a…

高能天体物理现象 · 物理学 2022-09-07 Yu-Peng Chen , Shu Zhang , Long Ji , Shuang-Nan Zhang , Ling-Da Kong , Peng-Ju Wang , Zhi Chang , Jing-Qiang Peng , Jian Li , Jin-Lu Qu

KS 1741-293 is a transient neutron star low-mass X-ray binary that is located at an angular distance of ~20' from the Galactic center. We map out the historic activity of the source since its discovery in 1989, characterize its most recent…

高能天体物理现象 · 物理学 2015-06-11 N. Degenaar , R. Wijnands

The high mass X-ray binary system 4U 0114+65 was observed by Nustar in October 2019, and by XMM-Newton in August 2015. Here we performed spectral and timing analysis of the Nustar observation, and carry out timing analysis on the XMM-Newton…

高能天体物理现象 · 物理学 2023-05-04 Mohammed H. Abdallah , Rasha M. Samir , Denis A. Leahy , Ashraf A. Shaker

Thermonuclear (type-I) X-ray bursts, observed from neutron star (NS) low-mass X-ray binaries (LMXB), provide constraints on NS masses and radii and consequently the equation of state of NS cores. In such analyses various assumptions are…

高能天体物理现象 · 物理学 2017-09-13 J. J. E. Kajava , K. I. I. Koljonen , J. Nättilä , V. Suleimanov , J. Poutanen

We present spectral and temporal properties of all the thermonuclear X-ray bursts observed from Aql X-1 by the Neutron Star Interior and Composition Explorer (NICER) between 2017 July and 2021 April. This is the first systematic…

We report the discovery of millisecond oscillations in an X-ray burst from the X-ray transient SAX J1748.9-2021 in the globular cluster NGC 6440. Oscillations at a frequency of 409.7 +/- 0.3 Hz were present in one of nine X-ray bursts…

天体物理学 · 物理学 2009-11-07 P. Kaaret , J. J. M. in 't Zand , J. Heise , J. A. Tomsick

The discovery of a type I X-ray burst from the faint unidentified transient source IGR J17445-2747 in the Galactic bulge by the JEM-X telescope onboard the INTEGRAL observatory is reported. Type I bursts are believed to be associated with…

高能天体物理现象 · 物理学 2017-09-11 I. A. Mereminskiy , S. A. Grebenev , R. A. Sunyaev

Spectral measurements of thermonuclear (type-I) X-ray bursts from low mass X-ray binaries have been used to measure neutron star (NS) masses and radii. A number of systematic issues affect such measurements and have raised concerns as to…

We present an analysis of the RXTE observations of 4U 1630-47 during its outburst of 1998. The light curve and the spectral evolution of the outburst were distinctly different from the outbursts of the same source in 1996 and in 1999.…

天体物理学 · 物理学 2009-10-31 Sergey P. Trudolyubov , Konstantin N. Borozdin , William C. Priedhorsky

We report on the results of a four-year long X-ray monitoring campaign of the central 1.2 square degrees of our Galaxy, performed with Chandra and XMM-Newton between 2005 and 2008. Our study focuses on the properties of transient X-ray…

高能天体物理现象 · 物理学 2015-06-04 N. Degenaar , R. Wijnands , E. M. Cackett , J. Homan , J. J. M. in 't Zand , E. Kuulkers , T. J. Maccarone , M. van der Klis

Superbursts were discovered at the beginning of this millennium. Just like type-I X-ray bursts, they are thought to be due to thermonuclear shell flashes on neutron stars, only igniting much deeper. With respect to type-I bursts, they last…

高能天体物理现象 · 物理学 2017-02-17 Jean in 't Zand

We searched for thermonuclear X-ray bursts from Galactic neutron stars in all event mode data of the Neil Gehrels Swift Observatory collected until March 31, 2018. In particular, we are interested in the intermediate-duration bursts (shell…

高能天体物理现象 · 物理学 2019-01-16 J. J. M. in 't Zand , M. J. W. Kries , D. M. Palmer , N. Degenaar

The neutron star binary SAX J1747.0-2853, located in the Galactic Center region at about 0.5 deg from Sgr A* and at a distance of 9 kpc, has been observed in outburst four times (1998, 1999, 2000 and 2001) by BeppoSAX and RossiXTE. At the…

天体物理学 · 物理学 2009-11-10 L. Natalucci , A. Bazzano , M. Cocchi , P. Ubertini , R. Cornelisse , J. Heise , J. J. M. in 't Zand

Thermonuclear flashes of hydrogen and helium accreted onto neutron stars produce the frequently observed Type I X-ray bursts. It is the current paradigm that almost all material burns in a burst, after which it takes hours to accumulate…

高能天体物理现象 · 物理学 2017-06-28 L. Keek , A. Heger

The Be/X-ray transient 4U 0115+63 exhibited a giant, type-II outburst in October 2015. The source did not decay to its quiescent state but settled in a meta-stable plateau state (a factor ~10 brighter than quiescence) in which its…

We present results from an observation of the Low Mass X-ray Binary 4U 1636-536 obtained with the LAXPC instrument aboard AstroSat. The observations of 4U 1636-536 made during the performance verification phase of AstroSat showed seven…

We present the results obtained from the spectral and temporal study of thermonuclear bursts from the millisecond X-ray pulsar SRGA J144459.2-604207 detected with NICER. The dynamic evolution of the spectral parameters in a broad energy…

高能天体物理现象 · 物理学 2025-07-23 Manoj Mandal , Sachindra Naik , Birendra Chhotaray

For the first time X-ray bursts have been detected from a sky position consistent with the one of GRS 1741.9-2853, a GRANAT transient source located only ~10' from the Galactic Centre. A total of 3 bursts have been observed by the Wide…

天体物理学 · 物理学 2007-05-23 M. Cocchi , A. Bazzano , L. Natalucci , P. Ubertini , J. Heise , J. M. Muller , J. J. M. in 't Zand

Two flares with a duration of several hours are reported for the low-mass X-ray binary 4U 1636-53. The characteristics of these flares (i.e., decay time scales, spectral softening, fluences) are very similar to the very long type-I X-ray…

天体物理学 · 物理学 2009-11-06 Rudy Wijnands

We present a detailed spectro-polarimetric study of Black hole X-ray binary 4U $1630-47$ during its $2022$ outburst with IXPE and NICER observations. The source is observed in disk dominated thermal state (kT$_{in}\approx1.4$ keV) with…

高能天体物理现象 · 物理学 2023-06-14 Ankur Kushwaha , Kiran M. Jayasurya , Vivek K. Agrawal , Anuj Nandi