Tidal disruption events as a site of an evolving relativistic spectral line
Author:
Affiliation:
1. Astronomical Institute, Faculty of Mathematics and PhysicsCharles University Prague Czech Republic
2. Astronomical InstituteCzech Academy of Sciences Prague Czech Republic
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.201913658
Reference32 articles.
1. The evolution of viscous discs - I. Mass transfer variations
2. IRON LINE PROFILES FROM RELATIVISTIC ELLIPTICAL ACCRETION DISKS
3. Cummings J. R. Barthelmy S. D. Beardmore A. P.et al.2011 GRB Coordinates Network Circular Service No. 11823 #1 (2011) 11823. Retrieved fromhttp://adsabs.harvard.edu/abs/2011GCN.11823.1C
4. A Unified Model for Tidal Disruption Events
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1. Spectral energy distribution profiles from AGN accretion disc in multigap set-up;Monthly Notices of the Royal Astronomical Society;2023-04-21
2. Light-curve Evolution of the Nearest Tidal Disruption Event: A Late-time, Radio-only Flare;The Astrophysical Journal;2022-02-01
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