Long-term pulse period evolution of the ultra-luminous X-ray pulsar NGC 7793 P13 (2021)
Attributed to:
Supermassive black hole growth - a small-scale solution to a large-scale problem
funded by
STFC
Abstract
No abstract provided
Bibliographic Information
Digital Object Identifier: http://dx.doi.org/10.1051/0004-6361/202140625
Publication URI: http://dx.doi.org/10.1051/0004-6361/202140625
Type: Journal Article/Review
Parent Publication: Astronomy & Astrophysics