EQUILIBRIUM MODELS FOR STARS WHICH DERIVE ENERGY FROM HELIUM-BURNING. I. STARS COMPOSED OF PURE HELIUM

Journal Article · Mon May 01 00:00:00 EDT 1961 · Astrophysical Journal (U.S.)

DOI:https://doi.org/10.1086/147081· OSTI ID:4028993

Cox, J P; Giuli, R T

• Research Organization: Cornell Univ., Ithaca, N.Y.
• NSA Number: NSA-15-024181
• OSTI ID: 4028993
• Journal Information: Astrophysical Journal (U.S.), Vol. Vol: 133; Other Information: Orig. Receipt Date: 31-DEC-61
• Country of Publication: Country unknown/Code not available
• Language: English

Related Subjects

PHYSICS
ALPHA PARTICLES
ASTROPHYSICS
COMPUTERS
ELECTRONS
EMISSION
ENERGY
HELIUM
HIGH TEMPERATURE
INTERACTIONS
LIGHT
MASS
NUMERICALS
PARTICLE MODELS
PRESSURE
PRODUCTION
RADIATIONS
SCATTERING
STARS
TEMPERATURE
THERMONUCLEAR REACTIONS