A Potential Cyclotron Resonant Scattering Feature in the Ultraluminous X-Ray Source Pulsar NGC 300 ULX1 Seen by NuSTAR and XMM-Newton (2018)

First Author: Walton D
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/10.3847/2041-8213/aabadc

Publication URI: http://dx.doi.org/10.3847/2041-8213/aabadc

Type: Journal Article/Review

Parent Publication: The Astrophysical Journal

Issue: 1