Modeling changing‐look active galactic nuclei phenomenon in 1D using accretion disk instabilities
Author:
Affiliation:
1. Nicolaus Copernicus Astronomical Center (PAN) Warsaw Poland
2. Center for Theoretical Physics Polish Academy of Sciences Warsaw Poland
Funder
Ministerstwo Nauki i Szkolnictwa Wyższego
Publisher
Wiley
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://onlinelibrary.wiley.com/doi/pdf/10.1002/asna.20210065
Reference40 articles.
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5. Methods and results of an automatic analysis of a complete sample ofSwift-XRT observations of GRBs
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