Evidence for evolving accretion disc structure in 4U1957+115
Author:
Publisher
Oxford University Press (OUP)
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://academic.oup.com/mnras/article-pdf/306/3/701/11932604/306-3-701.pdf
Reference27 articles.
1. Accretion disks in low-mass X-ray binaries
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4. A 106 Day Period in the Nuclear Source X-8 in M33
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1. IXPE observation confirms a high spin in the accreting black hole 4U 1957+115;Astronomy & Astrophysics;2024-04
2. First X-Ray Polarization Measurement Confirms the Low Black Hole Spin in LMC X-3;The Astrophysical Journal;2023-12-18
3. NICER/NuSTAR Characterization of 4U 1957+11: A Near Maximally Spinning Black Hole Potentially in the Mass Gap;The Astrophysical Journal;2023-02-01
4. Spectral characteristics of the black hole binary 4U 1957+115: a multi mission perspective;Monthly Notices of the Royal Astronomical Society;2022-10-16
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