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相关论文: Simultaneous NICER and NuSTAR Observations of the …

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The detection of coherent X-ray pulsations at ~314 Hz (3.2 ms) classifies MAXI J1957+032 as a fast-rotating, accreting neutron star. We present the temporal and spectral analysis performed using NICER observations collected during the…

We present X-ray spectral analyses for three Seyfert 2 active galactic nuclei, NGC 424, NGC 1320, and IC 2560, observed by NuSTAR in the 3-79 keV band. The high quality hard X-ray spectra allow detailed modeling of the Compton reflection…

We report the detection of a long X-ray burst triggered on MJD 60171.65 from the ultra-compact binary 4U 1850$-$087 by the Monitor of All-sky X-ray Image and Neutron Star Interior Composition Explorer (NICER). We analyse the NICER data…

高能天体物理现象 · 物理学 2024-07-31 Yongqi Lu , Zhaosheng Li , Wenhui Yu , Yuanyue Pan , Maurizio Falanga

We present results from a deep, coordinated $XMM$-$Newton$+$NuSTAR$ observation of the Seyfert 2 galaxy IRAS 00521-7054. The $NuSTAR$ data provide the first detection of this source in high-energy X-rays ($E > 10$ keV), and the broadband…

高能天体物理现象 · 物理学 2019-01-23 D. J. Walton , E. Nardini , L. C. Gallo , M. T. Reynolds , C. Ricci , T. Dauser , A. C. Fabian , J. A. Garcia , F. A. Harrison , G. Risaliti , D. Stern

Accretion disks and coronae around massive black holes have been studied extensively, and they are known to be coupled. Over a period of 30 years, however, the X-ray (coronal) flux of Mrk 817 increased by a factor of 40 while its UV (disk)…

The X-ray burster 4U1850-087, located in the globular cluster NGC6712, is an ultracompact binary likely harbouring a degenerate companion.The source has been observed with INTEGRAL several times, during the monitoring of the Galactic plane,…

天体物理学 · 物理学 2007-05-23 Lara Sidoli , Ada Paizis , Angela Bazzano , Sandro Mereghetti

We report the broadband spectro-temporal study of the poorly studied accreting neutron star (NS) low mass X-ray binary (LMXB) 4U 1724-30 using data from Soft X-ray Telescope (SXT) and Large Area X-ray Proportional Counters (LAXPC)…

高能天体物理现象 · 物理学 2022-04-13 Unnati Kashyap , Manoneeta Chakraborty , Sudip Bhattacharyya

We study the appearance of the neutron star - accretion disk system as seen by a distant observer in the UV/X-ray domain. The observed intensity spectra are computed assuming non-spherical geometry of the whole system, in which outgoing…

高能天体物理现象 · 物理学 2018-10-24 A. Rozanska , B. Beldycki , J. Madej , T. P. Adhikari , B. You

We report on the X-ray monitoring programme (covering slightly more than 11 days) carried out jointly by XMM-Newton and NuSTAR on the intermediate Seyfert galaxy Mrk 915. The light curves extracted in different energy ranges show a…

高能天体物理现象 · 物理学 2017-07-26 L. Ballo , P. Severgnini , R. Della Ceca , V. Braito , S. Campana , A. Moretti , C. Vignali , A. Zaino

We report the discovery of several optical burst-like events from the low-mass X-ray binary MS1603.6+2600 (UW CrB). The events last for a few tens of seconds, exhibit a very fast rise and slow decay, and involve optical brightening of a…

天体物理学 · 物理学 2009-11-10 R. I. Hynes , E. L. Robinson , E. Jeffery

We study X-ray and soft gamma-ray spectra from the hard state of the accreting black-hole binary MAXI J1820+070. We perform analysis of joint spectra from HXMT, NuSTAR and INTEGRAL. We find an overall agreement between the spectra from all…

高能天体物理现象 · 物理学 2022-03-30 Andrzej A. Zdziarski , Bei You , Michal Szanecki , Xiao-Bo Li , Min-Yu Ge

It is thought that ultraluminous X-ray sources (ULXs) are mainly powered by super-Eddington accreting neutron stars or black holes as shown by recent discovery of X-ray pulsations and relativistic winds. This work presents a follow up study…

The supernova impostor SN 2010da located in the nearby galaxy NGC 300, later identified as a likely supergiant B[e] high-mass X-ray binary, was simultaneously observed by NuSTAR and XMM-Newton between 2016 December 16 and 20, over a total…

高能天体物理现象 · 物理学 2018-03-14 S. Carpano , F. Haberl , C. Maitra , G. Vasilopoulos

We present the analysis of four NuSTAR observations of the luminous infrared galaxy merger NGC 6240, hosting a close pair of highly obscured active galactic nuclei (AGN). Over a period of about two years, the source exhibits hard X-ray…

高能天体物理现象 · 物理学 2017-08-23 Emanuele Nardini

A mysterious absorption feature at approximately 3.8 keV has been identified in the NICER spectrum of the low-mass X-ray binary system 4U 1820-30. We interpret this feature as a gravitationally redshifted iron absorption line. This…

高能天体物理现象 · 物理学 2025-11-26 R. Iaria , T. Di Salvo , A. Anitra , F. Barra , A. Sanna , C. Maraventano , C. Miceli , W. Leone , L. Burderi

We study the mass transfer rates and disk stability conditions of ultracompact X-ray binaries (UCXBs) using empirical time-averaged X-ray luminosities from Paper I (Cartwright et al. 2013) and compiled information from the literature. The…

高能天体物理现象 · 物理学 2015-06-15 C. O. Heinke , N. Ivanova , M. C. Engel , K. Pavlovskii , G. R. Sivakoff , T. F. Cartwright , J. C. Gladstone

The recent discovery of periodic pulsations from several members of the ultraluminous X-ray source (ULX) family in nearby galaxies as well as in our own galaxy unveiled the nature of the accreting compact object. Neutron stars rather than…

高能天体物理现象 · 物理学 2022-01-13 Mehmet Hakan Erkut

We present the detection of 51 thermonuclear X-ray bursts observed from 4U 1636-536 by the Neutron Star Interior Composition Explorer (NICER) over the course of a three year monitoring campaign. We performed time resolved spectroscopy for…

We perform a comprehensive study of thermonuclear bursts from the neutron star low-mass X-ray binary 4U 1702-429 detected with NICER and XMM-Newton. The thermonuclear burst detected with NICER shows clear evidence of a photospheric radius…

高能天体物理现象 · 物理学 2025-08-19 Manoj Mandal , Sachindra Naik , Gaurava Kumar Jaisawal

Based on new Chandra X-ray telescope data, we present empirical evidence of plasma Compton cooling during a flare in the non pulsating massive X-ray binary 4U1700-37. This behaviour might be explained by quasispherical accretion onto a…

高能天体物理现象 · 物理学 2017-12-06 M. Martinez-Chicharro , J. M. Torrejón , L. Oskinova , F. Fürst , K. Postnov , J. J. Rodes-Roca , R. Hainich , A. Bodaghee
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