An Evolving Broad Iron Line from the First Galactic Ultraluminous X-Ray Pulsar Swift J0243.6+6124-Reference-Cited by-同舟云学术

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

Published:2019-10-25 Issue:1 Volume:885 Page:18
ISSN:1538-4357
Container-title:The Astrophysical Journal
language:
Short-container-title:ApJ

Author:

Jaisawal Gaurava K.^ORCID,Wilson-Hodge Colleen A.^ORCID,Fabian Andrew C.^ORCID,Naik Sachindra^ORCID,Chakrabarty Deepto^ORCID,Kretschmar Peter^ORCID,Ballantyne David R.^ORCID,Ludlam Renee M.^ORCID,Chenevez Jérôme^ORCID,Altamirano Diego^ORCID,Arzoumanian Zaven,Fürst Felix^ORCID,Gendreau Keith C.,Guillot Sebastien^ORCID,Malacaria Christian^ORCID,Miller Jon M.,Stevens Abigail L.,Wolff Michael T.^ORCID

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Link

https://iopscience.iop.org/article/10.3847/1538-4357/ab4595/pdf

Reference60 articles.

1. An ultraluminous X-ray source powered by an accreting neutron star

2. IONIZED REFLECTION SPECTRA FROM ACCRETION DISKS ILLUMINATED BY X-RAY PULSARS

3. Rotating Black Holes: Locally Nonrotating Frames, Energy Extraction, and Scalar Synchrotron Radiation

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