An Evolving Broad Iron Line from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

An Evolving Broad Iron Line from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124

We present a spectral study of the ultraluminous Be/X-ray transient pulsar Swift J0243.6+6124 using Neutron Star Interior Composition Explorer (NICER) observations during the system's 2017-2018 giant outburst. The 1.2-10 keV energy spectrum of the source can be approximated with an absorbed cut...

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Bibliographic Details
Main Authors: Jaisawal, Gaurava K., Wilson-Hodge, Colleen A., Fabian, Andrew C., Naik, Sachindra, Chakrabarty, Deepto, Kretschmar, Peter, Ballantyne, David R., Ludlam, Renee M., Chenevez, Jérôme, Altamirano, Diego, Arzoumanian, Zaven, Fürst, Felix, Gendreau, Keith C., Guillot, Sebastien, Malacaria, Christian, Miller, Jon M., Stevens, Abigail L., Wolff, Michael T.
Other Authors: MIT Kavli Institute for Astrophysics and Space Research
Format: Article
Language:English
Published: American Astronomical Society 2021
Online Access:https://hdl.handle.net/1721.1/129696

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https://hdl.handle.net/1721.1/129696

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