Rimmed and Rippled Accretion Disc Models to Explain AGN Continuum Lags (2022)
Attributed to:
Astronomy at St Andrews 2015-2018
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.2212.01379
Publication URI: https://arxiv.org/abs/2212.01379
Type: Other