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Discovery of a 2.8 s pulsar in a 2 d orbit High-Mass X-ray Binary powering the Ultraluminous X-ray source ULX-7 in M51 (2019)

First Author: Castillo G

Attributed to: A Programme of Astronomical Instrumentation and High-Energy Astrophysics at Durham 2013-2015 funded by STFC

Abstract

No abstract provided

Bibliographic Information

Digital Object Identifier: http://dx.doi.org/10.48550/arxiv.1906.04791

Publication URI: https://arxiv.org/abs/1906.04791

Type: Other