Pulsed Iron Line Emission from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

Autor: Y. X. Xiao, Y. J. Xu, M. Y. Ge, F. J. Lu, S. N. Zhang, S. Zhang, L. Tao, J. L. Qu, P. J. Wang, L. D. Kong, Y. L. Tuo, Y. You, S. J. Zhao, J. Q. Peng, Y. F. Du, Y. H. Zhang, W. T. Ye

Publikováno v: The Astrophysical Journal, Vol 965, Iss 1, p 18 (2024)

We report the phase-resolved spectral results of the first Galactic pulsating ultraluminous X-ray source (PULX) Swift J0243.6+6124, modeling its 2017–2018 outburst peak using data collected by the Hard X-ray Modulation Telescope (Insight-HXMT). The

Externí odkaz: https://doaj.org/article/207301a8b77c471a8c3a45ee824a2e7a

A possible overall scenario for the outburst evolution of MAXI J1820+070 revealed by Insight-HXMT

Autor: J Q Peng, S Zhang, Y P Chen, L D Kong, P J Wang, S N Zhang, L Ji, L Tao, J L Qu, M Y Ge, Q C Shui, J Li, Z Chang, Z S Li, Y X Xiao

Publikováno v: Monthly Notices of the Royal Astronomical Society. 518:2521-2528

We study the spectral and temporal properties of the black hole X-ray transient binary MAXI J1820+070 during the 2018 outburst with Insight-HXMT observations. The outburst of MAXI J1820+070 can be divided into three intervals. For the two intervals o

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::085b43cec8d4421ab3ed530b92cc2f7b
https://doi.org/10.1093/mnras/stac3238

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The 2018 failed outburst of H 1743 – 322: Insight-HXMT, NuSTAR, and NICER views

Autor: P J Wang, L D Kong, Y P Chen, S Zhang, S N Zhang, R Soria, L Ji, J L Qu, Y Huang, L Tao, M Y Ge, F J Lu, L Chen, T P Li, Y P Xu, X L Cao, Y Chen, C Z Liu, Q C Bu, C Cai, Z Chang, T X Chen, Y B Chen, W W Cui, Y Y Du, G H Gao, H Gao, Y D Gu, J Guan, C C Guo, D W Han, J Huo, S M Jia, W C Jiang, J Jin, B Li, C K Li, G Li, W Li, X Li, X B Li, X F Li, Z W Li, X H Liang, J Y Liao, B S Liu, H X Liu, H W Liu, X J Liu, X F Lu, Q Luo, T Luo, R C Ma, X Ma, B Meng, Y Nang, J Y Nie, G Ou, X Q Ren, N Sai, L M Song, X Y Song, L Sun, Y Tan, Y L Tuo, C Wang, L J Wang, W S Wang, Y S Wang, X Y Wen, B Y Wu, B B Wu, M Wu, G C Xiao, S Xiao, S L Xiong, R J Yang, S Yang, Yan Ji Yang, Yi Jung Yang, Q B Yi, Q Q Yin, Y You, F Zhang, H M Zhang, J Zhang, P Zhang, W C Zhang, W Zhang, Y F Zhang, Y H Zhang, H S Zhao, X F Zhao, S J Zheng, Y G Zheng, D K Zhou

Publikováno v: Monthly Notices of the Royal Astronomical Society. 512:4541-4555

We studied the 2018 outburst of the black hole transient H 1743 − 322 with a series of Insight-HXMT, NICER, and NuSTAR observations, covering the 1–120 keV band. With our broad-band X-ray spectral modelling, we confirm that the source remained in

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=doi_________::8274eef826abbaa57ae568ce1f6c2f65
https://doi.org/10.1093/mnras/stac773