Steady-state nuclear fusion in accreting neutron-star envelopes

• 1 February 1975
• journal article
• Published by American Astronomical Society in The Astrophysical Journal
• Vol. 195, 735-741
• https://doi.org/10.1086/153375

Abstract

Keywords

• ASTRONOMICAL MODELS
• NEUTRON STARS
• NUCLEAR ASTROPHYSICS
• NUCLEAR FUSION
• STELLAR ENVELOPES
• STELLAR EVOLUTION
• X RAY SOURCES
• BINARY STARS
• COMPUTERIZED SIMULATION
• HELIUM
• HYDROGEN
• STEADY STATE
• THERMAL INSTABILITY
• X RAY STARS