Physical origin of the non-physical spin evolution of MAXI J1820 + 070

ABSTRACT We report on the Insight-HXMT observations of the new black hole X-ray binary MAXI J1820+070 during its 2018 outburst. Detailed spectral analysis via the continuum fitting method shows an evolution of the inferred spin during its high soft sate. Moreover, the hardness ratio, the non-thermal...

Full description

Bibliographic Details

Published in:	Monthly notices of the Royal Astronomical Society 2021-06, Vol.504 (2), p.2168-2180
Main Authors:	Guan, J, Tao, L, Qu, J L, Zhang, S N, Zhang, W, Zhang, S, Ma, R C, Ge, M Y, Song, L M, Lu, F J, Li, T P, Xu, Y P, Chen, Y, Cao, X L, Liu, C Z, Zhang, L, Wang, Y N, Chen, Y P, Bu, Q C, Cai, C, Chang, Z, Chen, L, Chen, T X, Chen, Y B, Cui, W W, Du, Y Y, Gao, G H, Gao, H, Gu, Y D, Guo, C C, Han, D W, Huang, Y, Huo, J, Jia, S M, Jiang, W C, Jin, J, Kong, L D, Li, B, Li, C K, Li, G, Li, W, Li, X, Li, X B, Li, X F, Li, Z W, Liang, X H, Liao, J Y, Liu, B S, Liu, H W, Liu, H X, Liu, X J, Lu, X F, Luo, Q, Luo, T, Ma, X, Meng, B, Nang, Y, Nie, J Y, Ou, G, Ren, X Q, Sai, N, Song, X Y, Sun, L, Tan, Y, Wang, C, Wang, L J, Wang, P J, Wang, W S, Wang, Y S, Wen, X Y, Wu, B B, Wu, B Y, Wu, M, Xiao, G C, Xiao, S, Xiong, S L, Yang, R J, Yang, S, Yang, Y J, Yi, Q B, Yin, Q Q, You, Y, Zhang, F, Zhang, H M, Zhang, J, Zhang, P, Zhang, W C, Zhang, Y F, Zhang, Y H, Zhao, H S, Zhao, X F, Zheng, S J, Zheng, Y G, Zhou, D K
Format:	Article
Language:	English
Subjects:	Accretion disks Black holes Circular orbits Evolution Luminosity Orbital stability Spectrum analysis Spin transition X ray binaries X ray stars
Citations:	Items that this one cites Items that cite this one
Online Access:	Request full text
Tags:	Add Tag No Tags, Be the first to tag this record!