Synchrotron afterglow model for AT 2022cmc: jetted tidal disruption event or engine-powered supernova?
Author:
Affiliation:
1. Department of Physics and Columbia Astrophysics Laboratory, Columbia University , Pupin Hall, New York, NY 10027 , USA
2. Center for Computational Astrophysics, Flatiron Institute , 162 5th Avenue, New York, NY 10010 , USA
Abstract
Funder
JSPS
National Science Foundation
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/stad1182/50064449/stad1182.pdf
Reference103 articles.
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3. A CONTINUUM OF H- TO He-RICH TIDAL DISRUPTION CANDIDATES WITH A PREFERENCE FOR E+A GALAXIES
4. Type I supernovae. I - Analytic solutions for the early part of the light curve
5. ON THE ORIGIN OF THE RADIO EMISSION OF Sw 1644+57
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1. Ultra high energy cosmic rays from tidal disruption events;Journal of Cosmology and Astroparticle Physics;2023-11-01
2. A Unified Theory of Jetted Tidal Disruption Events: From Promptly Escaping Relativistic to Delayed Transrelativistic Jets;The Astrophysical Journal Letters;2023-10-30
3. Swift J1644+57 as an off-axis Jet;Monthly Notices of the Royal Astronomical Society;2023-06-28
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