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Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51 (2020)

First Author: Rodríguez Castillo G

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/ab8a44

Publication URI: http://dx.doi.org/10.3847/1538-4357/ab8a44

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1