Relation of Cyclotron Resonant Energy and Luminosity in a Strongly Magnetized Neutron Star GRO J1008-57 Observed by Insight-HXMT
Author:
Funder
National Natural Science Foundation of China
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.3847/1538-4357/ac1268/pdf
Reference56 articles.
1. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
2. Dynamical Structure of Radiation‐dominated Pulsar Accretion Shocks
3. Spectral formation in accreting X-ray pulsars: bimodal variation of the cyclotron energy with luminosity
4. CONFIRMATION OF A HIGH MAGNETIC FIELD IN GRO J1008–57
5. On timing and spectral characteristics of the X-ray pulsar 4U 0115+63: Evolution of the pulsation period and the cyclotron line energy
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