Spectral fit of Cygnus X-1 in high energy— a self-consistent study
Author:
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://link.springer.com/content/pdf/10.1007/s10509-007-9438-3.pdf
Reference12 articles.
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2. Chakrabarti, S.K., Mandal, S.: Spectral properties of shocked accretion flows—a self-consistent study. Astron. Space Sci., doi: 10.1007/s10509-007-9398-7 (2007)
3. Chakrabarti, S.K., Titarchuk, L.G.: Spectral properties of accretion disks around galactic and extragalactic black holes. Astrophys. J. 455, 623 (1995)
4. Ebisawa, K., Titarchuk, L.G., Chakrabarti, S.K.: On the spectral slopes of hard X-ray emission from black hole candidates. Publ. Astron. Soc. Jpn. 48, 59 (1996)
5. Ling, J.C., Wheaton, W.A.: BATSE soft gamma-ray observations of GRO J0422+32. Astrophys. J. 584, 399 (2003)
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1. On the origin of core radio emissions from black hole sources in the realm of relativistic shocked accretion flow;Monthly Notices of the Royal Astronomical Society;2022-05-20
2. AstroSat and MAXI view of Cygnus X-1: Signature of an ‘extreme’ soft nature;Monthly Notices of the Royal Astronomical Society;2021-08-05
3. Clumpy Wind Accretion in Cygnus X-1;The Astrophysical Journal;2020-11-01
4. Spectral properties of shocked accretion flows— a self-consistent study;Astrophysics and Space Science;2007-04-19
5. Spectral properties of shocked accretion flows— a self-consistent study;The Multi-Messenger Approach to High-Energy Gamma-Ray Sources;2007
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