Swift Monitoring of M51: A 38 day Superorbital Period for the Pulsar ULX7 and a New Transient Ultraluminous X-Ray Source (2020)

First Author: Brightman M
Attributed to:  Black Holes and Accretion: Observational Frontiers funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.3847/1538-4357/ab7e2a

Publication URI: http://dx.doi.org/10.3847/1538-4357/ab7e2a

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 2