Numerical models of neutron star atmospheres from fusion ashes show a radiation-pressure layer limiting flux and absorption edges tied to chemical composition, with fits to diluted blackbodies plus edges for X-ray burst interpretation.
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Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.
citing papers explorer
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Neutron star atmospheres composed of fusion ashes
Numerical models of neutron star atmospheres from fusion ashes show a radiation-pressure layer limiting flux and absorption edges tied to chemical composition, with fits to diluted blackbodies plus edges for X-ray burst interpretation.
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The compact neutron star in 4U 1746-37 revisited: Reassessing the mass and radius
Significant X-ray flux blocking in 4U 1746-37 allows the neutron star to have canonical mass and radius values of 1.59 solar masses and 13 km or 2.12 solar masses and 9.8 km.