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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: Astronomy Observation and Theory Consolidated Grant 2016-2019 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 Letters

Issue: 1