Ultra-luminous X-Ray Sources as Super-critical Propellers
Author:
Publisher
American Astronomical Society
Subject
Space and Planetary Science,Astronomy and Astrophysics
Link
http://stacks.iop.org/0004-637X/873/i=2/a=105/pdf
Reference70 articles.
1. On Young Neutron Stars as Propellers and Accretors with Conventional Magnetic Fields
2. An ultraluminous X-ray source powered by an accreting neutron star
3. Formation and evolution of binary and millisecond radio pulsars
4. Neutron star accretion and binary pulsar formation
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1. Statistical study of a large and cleaned sample of ultraluminous and hyperluminous X-ray sources;Astronomy & Astrophysics;2024-01
2. Evolution of fallback discs around millisecond magnetars: effect of supercritical accretion on GRB afterglows;Monthly Notices of the Royal Astronomical Society;2023-09-01
3. Probing the nature of the low state in the extreme ultraluminous X-ray pulsar NGC 5907 ULX1;Astronomy & Astrophysics;2023-04
4. Propeller states in locally supercritical ULXs;Monthly Notices of the Royal Astronomical Society;2022-12-21
5. Study on the magnetic field strength of NGC 300 ULX1;Monthly Notices of the Royal Astronomical Society;2022-05-17
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