X-ray polarization changes with the state transition in Cygnus X–1
Author:
Affiliation:
1. Institute of Astronomy, National Tsing Hua University , Hsinchu 300044 , Taiwan
2. Instituto de Estudios Astrofísicos, Facultad de Ingeniería y Ciencias, Universidad Diego Portales , Av. Ejército Libertador 441, Santiago , Chile
Abstract
Funder
Ministry of Science and Technology of Taiwan
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://academic.oup.com/mnras/advance-article-pdf/doi/10.1093/mnras/stad3961/54770898/stad3961.pdf
Reference52 articles.
1. ixpeobssim: A simulation and analysis framework for the imaging X-ray polarimetry explorer
2. Analysis of NuSTAR and Suzaku observations of Cyg X-1 in the hard state: evidence for a truncated disc geometry
3. Spectral Properties of Accretion Disks around Galactic and Extragalactic Black Holes
4. Images and spectral properties of two-component advective flows around black holes: effects of photon bending
Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献
1. Polarized X-rays correlated with the short-timescale variability of Cygnus X-1;Publications of the Astronomical Society of Japan;2024-07-25
2. An IXPE-led X-Ray Spectropolarimetric Campaign on the Soft State of Cygnus X-1: X-Ray Polarimetric Evidence for Strong Gravitational Lensing;The Astrophysical Journal Letters;2024-07-01
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