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25 April 2024
 
  » arxiv » 1912.8542

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Diagnostic of the spectral properties of Aquila X-1 by Insight-HXMT snapshots during the early propeller phase
C. Güngör ; M. Y. Ge ; S. Zhang ; A. Santangelo ; S. N. Zhang ; F. J. Lu ; Y. Zhang ; Y. P. Chen ; L. Tao ; Y. J. Yang ; Q. C. Bu ; C. Cai ; X. L. Cao ; Z. Chang ; G. Chen ; L. Chen ; T. X. Chen ; Y. Chen ; Y. B. Chen ; W. Cui ; W. W. Cui ; J. K. Deng ; Y. W. Dong ; Y. Y. Du ; M. X. Fu ; G. H. Gao ; H. Gao ; M. Gao ; Y. D. Gu ; J. Guan ; C. C. Guo ; D. W. Han ; Y. Huang ; J. Huo ; L. Ji ; S. M. Jia ; L. H. Jiang ; W. C. Jiang ; J. Jin ; L. D. Kong ; B. Li ; C. K. Li ; G. Li ; M. S. Li ; T. P. Li ; W. Li ; X. Li ; X. B. Li ; X. F. Li ; Y. G. Li ; Z. W. Li ; X. H. Liang ; J. Y. Liao ; C. Z. Liu ; G. Q. Liu ; H. W. Liu ; X. J. Liu ; Y. N. Liu ; B. Lu ; X. F. Lu ; T. Luo ; Q. Luo ; X. Ma ; B. Meng ; Y. Nang ; J. Y. Nie ; G. Ou ; N. Sai ; L. M. Song ; X. Y. Song ; L. Sun ; Y. Tan ; Y. L. Tuo ; C. Wang ; G. F. Wang ; J. Wang ; W. S. Wang ; Y. S. Wang ; X. Y. Wen ; B. B. Wu ; B. Y. Wu ; M. Wu ; G. C. Xiao ; S. Xiao ; S. L. Xiong ; Y. P. Xu ; J. W. Yang ; S. Yang ; Y. J. Yang ; Q. B. Yi ; Q. Q. Yin ; Y. You ; A. M. Zhang ; C. M. Zhang ; F. Zhang ; H. M. Zhang ; J. Zhang ; T. Zhang ; W. Zhang ; W. C. Zhang ; W. Z. Zhang ; Y. Zhang ; Y. F. Zhang ; Y. J. Zhang ; Z. Zhang ; Z. L. Zhang ; H. S. Zhao ; X. F. Zhao ; S. J. Zheng ; D. K. Zhou ; J. F. Zhou ; Y. Zhu ; Y. X. Zhu ;
Date 18 Dec 2019
AbstractWe study the 2018 outburst of Aql X-1 via the monitor of all sky X-ray image (MAXI) data. We show that the outburst starting in February 2018 is a member of short-low class in the frame of outburst duration and the peak count rate although the outburst morphology is slightly different from the other fast-rise-exponential-decay (FRED) type outbursts with a milder rising stage. We study the partial accretion in the weak propeller stage of Aql X-1 via the MAXI data of the 2018 outburst. We report on the spectral analysis of 3 observations of Aquila X-1 obtained by Insight - hard X-ray modulation telescope (Insight-HXMT) during the late decay stage of the 2018 outburst. We discuss that the data taken by Insight-HXMT is just after the transition to the weak propeller stage. Our analysis shows the necessity of a comptonization component to take into account the existence of an electron cloud resulting photons partly up-scattered.
Source arXiv, 1912.8542
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