THERMODYNAMICS UNDER CONDITIONS OF HOT MATTER NEUTRONIZATION AND THE HYDRODYNAMIC STABILITY OF STARS AT LATE STAGES OF EVOLUTION.

Journal Article · Fri Jan 01 00:00:00 EST 1971 · Sov. Astron. AJ (Engl. Transl.) 14: 747-57(Mar-Apr 1971).

OSTI ID:4007910

Imshennik, V S; Chechetkin, V M

• Research Organization: Inst. of Applied Mathematics, Moscow
• NSA Number: NSA-25-027335
• OSTI ID: 4007910
• Journal Information: Sov. Astron. AJ (Engl. Transl.) 14: 747-57(Mar-Apr 1971)., Other Information: Orig. Receipt Date: 31-DEC-71; Related Information: Translated from Astron. Zh.; 47: 929-41(Sep-Oct 1970).
• Country of Publication: Country unknown/Code not available
• Language: English

Related Subjects

N32120* -Physics-Astrophysics-Stars
ANTINEUTRINOS
DENSITY
EMISSION
MATTER
NEUTRINOS
STABILITY
STAR EVOLUTION
STARS
TEMPERATURE
THERMODYNAMICS
THERMONUCLEAR REACTIONS
ZONES
STARS/neutronization in central regions of
thermodynamics of hot matter
(T)
NEUTRINOS/emission from stars undergoing neutronization
(T)
STARS/stability at late evolutionary stages
hydrodynamic
(T)