Non-blackbody Disks Can Help Explain Inferred AGN Accretion Disk Sizes (2018)
Attributed to:
Astronomy at St Andrews 2018-2021
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/aaa768
Publication URI: http://dx.doi.org/10.3847/1538-4357/aaa768
Type: Journal Article/Review
Parent Publication: The Astrophysical Journal
Issue: 2