Properties of relativistic hot accretion flow around a rotating black hole with radially varying viscosity
Author:
Funder
Science and Engineering Research Board (SERB) of India
Publisher
Springer Science and Business Media LLC
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://link.springer.com/content/pdf/10.1007/s10509-023-04263-6.pdf
Reference82 articles.
1. Abramowicz, M.A., Chakrabarti, S.K.: Standing shocks in adiabatic black hole accretion of rotating matter. Astrophys. J. 350, 281 (1990). https://doi.org/10.1086/168380
2. Aktar, R., Das, S., Nandi, A., et al.: Estimation of mass outflow rates from dissipative accretion disc around rotating black holes. Mon. Not. R. Astron. Soc. 471(4), 4806–4819 (2017). https://doi.org/10.1093/mnras/stx1893. arXiv:1707.07511 [astro-ph.HE]
3. Aktar, R., Das, S., Nandi, A., et al.: Advective accretion flow properties around rotating black holes – application to GRO J1655-40. J. Astrophys. Astron. 39(1), 17 (2018). https://doi.org/10.1007/s12036-017-9507-0. arXiv:1801.04116 [astro-ph.HE]
4. Aktar, R., Nandi, A., Das, S.: Accretion-ejection in rotating black holes: a model for ‘outliers’ track of radio-X-ray correlation in X-ray binaries. Astrophys. Space Sci. 364(2), 22 (2019). https://doi.org/10.1007/s10509-019-3509-0. arXiv:1901.10091 [astro-ph.HE]
5. Baby, B.E., Agrawal, V.K., Ramadevi, M.C., et al.: AstroSat and MAXI view of the black hole binary 4U 1630-472 during 2016 and 2018 outbursts. Mon. Not. R. Astron. Soc. 497(1), 1197–1211 (2020). https://doi.org/10.1093/mnras/staa1965. arXiv:2007.00928 [astro-ph.HE]
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