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High plasma cut-off frequency blocks the radio emission from accreting millisecond X-ray pulsar SAX J1808.4-3658 期刊论文  OAI收割
Astrophysics and Space Science, 2020, 卷号: 365, 期号: 3, 页码: 47
作者:  Wang, S. Q.;  Zhang, C. M.;  Wang, D. H.;  Wang, N.;  Wang, J. B.
  |  收藏  |  浏览/下载：23/0  |  提交时间：2021/04/12
An underlying clock in the extreme flip-flop state transitions of the black hole transient Swift J1658.2-4242 期刊论文  OAI收割
Astronomy and Astrophysics, 2020, 卷号: 641, 页码: A101
作者:  HXMT
  |  收藏  |  浏览/下载：58/0  |  提交时间：2022/02/08
accretion  accretion disks  black hole physics  X-rays: binaries  time  Astrophysics - High Energy Astrophysical Phenomena  Abstract:
Aims: Flip-flops are top-hat-like X-ray flux variations, which have been observed in some transient accreting black hole binary systems, and feature simultaneous changes in the spectral hardness and the power density spectrum (PDS). They occur at a crucial time in the evolution of these systems, when the accretion disc emission starts to dominate over coronal emission. Flip-flops remain a poorly understood phenomenon, so we aim to thoroughly investigate them in a system featuring several such transitions.
Methods: Within the multitude of observations of Swift J1658.2-4242 during its outburst in early 2018, we detected 15 flip-flops, enabling a detailed analysis of their individual properties and the differences between them. We present observations by XMM-Newton, NuSTAR, Astrosat, Swift, Insight-HXMT, INTEGRAL, and ATCA. We analysed their light curves, searched for periodicities, computed their PDSs, and fitted their X-ray spectra, to investigate the source behaviour during flip-flop transitions and how the interval featuring flip-flops differs from the rest of the outburst.
Results: The flip-flops of Swift J1658.2-4242 are of an extreme variety, exhibiting flux differences of up to 77% within 100 s, which is much larger than what has been seen previously. We observed radical changes in the PDS simultaneous with the sharp flux variations, featuring transitions between the quasi-periodic oscillation types C and A, which have never been observed before. Changes in the PDS are delayed, but more rapid than changes in the light curve. Flip-flops occur in two intervals within the outburst, separated by about two weeks in which these phenomena were not seen. Transitions between the two flip-flop states occurred at random integer multiples of a fundamental period of 2.761 ks in the first interval and 2.61 ks in the second. Spectral analysis reveals the high and low flux flip-flop states to be very similar, but distinct from intervals lacking flip-flops. A change of the inner temperature of the accretion disc is responsible for most of the flux difference in the flip-flops. We also highlight the importance of correcting for the influence of the dust scattering halo on the X-ray spectra.  
Deprojection technique for galaxy cluster considering the point spread function 期刊论文  OAI收割
SCIENCE CHINA-PHYSICS MECHANICS & ASTRONOMY, 2010, 卷号: 53, 期号: 1, 页码: #REF!
作者:  Wang YS(王于仨);  Jia SM(贾淑梅);  Chen Y(陈勇);  Wang, YS;  Jia, SM
收藏  |  浏览/下载：12/0  |  提交时间：2016/04/12
Metal enrichment via ram pressure stripping in the IGM of the compact galaxy group RGH 80 期刊论文  OAI收割
RESEARCH IN ASTRONOMY AND ASTROPHYSICS, 2010, 卷号: 10, 期号: 4, 页码: 301
作者:  Cui HaiJuan;  Xu HaiGuang;  Gu JunHua;  Wang JingYing;  Gu LiYi
  |  收藏  |  浏览/下载：15/0  |  提交时间：2021/12/06
Determining the dust extinction of gamma-ray burst host galaxies: A direct method based on optical and X-ray photometry 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL  , 2008, 卷号: 678, 期号: 2, 页码: 1136-1141
Li Y.; Li Aigen; Wei D. M.
收藏  |  浏览/下载：19/0  |  提交时间：2011/12/30
Soft X-ray spectroscopy of highly charged silicon ions in dense plasmas 期刊论文  OAI收割
ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES, 2008, 卷号: 177, 期号: 1, 页码: 326
Liang, GY; Zhao, G; Zhong, JY; Li, YT; Liu, YQ; Dong, QL; Yuan, XH; Jin, Z; Zhang, J
收藏  |  浏览/下载：20/0  |  提交时间：2013/09/24
Extragalactic H(2)O masers and X-ray absorbing column densities 期刊论文  OAI收割
ASTRONOMY & ASTROPHYSICS  , 2006, 卷号: 450, 期号: 3, 页码: 933-U16
Zhang JS; Henkel C; Kadler M
收藏  |  浏览/下载：18/0  |  提交时间：2012/02/07
Properties of the diffuse X-ray background in a high-resolution hydrodynamical simulation 期刊论文  OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 卷号: 368, 期号: 1, 页码: 74-84
作者:  Dolag, K;  Roncarelli, M , Univ Bologna, Dipartimento Astron, Via Ranzani 1, I-40127 Bologna, Italy;  Murante, G;  Roncarelli, M;  Moscardini, L
  |  收藏  |  浏览/下载：19/0  |  提交时间：2012/08/02
Systematics in the X-ray cluster mass estimators 期刊论文  OAI收割
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, 2006, 卷号: 369, 期号: 4, 页码: 2013-2024
作者:  Rasia, E;  Ettori, S;  Moscardini, L;  Mazzotta, P;  Borgani, S
  |  收藏  |  浏览/下载：24/0  |  提交时间：2012/08/02