On the magnetic fields of ultraluminous X-ray pulsars
Author:
Publisher
IOP Publishing
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
https://iopscience.iop.org/article/10.1088/1674-4527/21/8/196/pdf
Reference65 articles.
1. An ultraluminous X-ray source powered by an accreting neutron star
2. All at Once: Transient Pulsations, Spin-down, and a Glitch from the Pulsating Ultraluminous X-Ray Source M82 X-2
3. The Limiting Luminosity of Accreting Neutron Stars With Magnetic Fields
4. Magnetic field strength of a neutron-star-powered ultraluminous X-ray source
5. Thomson Scattering in a Strong Magnetic Field
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1. Phase-dependent Spectral Shape Changes in the Ultraluminous X-Ray Pulsar NGC 5907 ULX1;The Astrophysical Journal;2024-06-01
2. Super-Eddington accretion as a possible scenario to form GW190425;Monthly Notices of the Royal Astronomical Society;2023-09-14
3. Probing the nature of the low state in the extreme ultraluminous X-ray pulsar NGC 5907 ULX1;Astronomy & Astrophysics;2023-04
4. Research on the Magnetic Field of NGC 7793 P13 and Other Confirmed Pulsating Ultraluminous X-Ray Sources;Research in Astronomy and Astrophysics;2022-11-01
5. Formation of mass-gap black holes from neutron star X-ray binaries with super-Eddington accretion;Monthly Notices of the Royal Astronomical Society;2022-05-25
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