The appearance of highly relativistic, spherically symmetric stellar winds

• 1 March 1991
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 369, 175-178
• https://doi.org/10.1086/169748

Abstract

Keywords

• NEUTRON STAR
• QUANTUM MECHANICS
• GENERAL RELATIVITY
• ATMOSPHERES
• NEUTRON STARS
• SCATTERING
• BINARY STARS
• FIELD THEORY
• PHYSICAL PROPERTIES
• RADIATIVE TRANSFER
• RELATIVITY THEORY
• STARS
• ELECTRON SCATTERING
• LORENTZ FORCE
• OPACITY
• STELLAR WINDS
• STELLAR ATMOSPHERES
• BINARY STAR
• STEADY STATE