EVOLUTION OF THE STARS

Journal Article · Mon Jan 01 00:00:00 EST 1962 · Progr. Theoret. Phys. (Kyoto), Suppl.

DOI:https://doi.org/10.1143/PTPS.22.1· OSTI ID:4124884

Hayashi, C; Hoshi, R; Sugimoto, D

Modern theories on the evolution of stars are extended to the phases of helium burning, carbon burning, and later burnings as far as possible, and the theoretical results are compared wth the Hertzsprung-Russell diagrams of star clusters. The topics discussed include nuclear generation and energy loss by neutrinos, quasi-static equilibrium, envelope,core, and surface solutions, stellar models with homogeneous chemical composition, hydrogen burning phase, helium burning phase, advanced phases of nuclear burning, iinal phase toward white dwarfs, and pre-mainsequence contricting phase. (C.E.S.)

• Research Organization: Kyoto Univ. (Japan)
• Sponsoring Organization: USDOE
• NSA Number: NSA-18-008990
• OSTI ID: 4124884
• Journal Information: Progr. Theoret. Phys. (Kyoto), Suppl., Vol. Vol: No. 22; Other Information: Orig. Receipt Date: 31-DEC-64
• Country of Publication: Country unknown/Code not available
• Language: English

Related Subjects

PHYSICS
ASTROPHYSICS
CARBON
CONFIGURATION
DIAGRAMS
ELEMENTS
ENERGY
HELIUM
LOSSES
NEUTRINOS
PARTICLE MODELS
PRODUCTION
QUANTITY RATIO
STAR CLUSTERS
STARS
SURFACES
THERMONUCLEAR REACTIONS
WHITE DWARFS