STELLAR EVOLUTION TOWARD PRE-SUPERNOVA STAGE .2. CARBON AND OXYGEN STARS OF 1.5M. AND 2.6M.

被引：16

作者：

IKEUCHI, S

NAKAZAWA, K

MURAI, T

HOSHI, R

HAYASHI, C

机构：

[1] KYOTO UNIV,DEPT PHYS,KYOTO,JAPAN

[2] NAGOYA UNIV,DEPT PHYS,NAGOYA,JAPAN

[3] RIKKYO UNIV,DEPT PHYS,TOKYO,JAPAN

来源：

PROGRESS OF THEORETICAL PHYSICS | 1972年 / 48卷 / 6A期

关键词：

D O I：

10.1143/PTP.48.1870

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

引用

页码：1870 / 1884

页数：15

共 23 条

[1] Arnet W. D., 1967, CAN J PHYS, V45, P1621
[2] GRAVITATIONAL COLLAPSE AND WEAK INTERACTIONS
ARNETT, WD
[J]. CANADIAN JOURNAL OF PHYSICS, 1966, 44 (11) : 2553 - +
[3] ENERGY LOSSES DUE TO NEUTRINO PROCESSES
BEAUDET, G
PETROSIAN, V
SALPETER, EE
[J]. ASTROPHYSICAL JOURNAL, 1967, 150 (3P1) : 979 - +
[4] Chandrasekhar S., 1961, HYDRODYNAMICS HYDROM
[5] HYDRODYNAMIC BEHAVIOR OF SUPERNOVAE EXPLOSIONS
COLGATE, SA
WHITE, RH
[J]. ASTROPHYSICAL JOURNAL, 1966, 143 (03) : 626 - &
[6] ADVANCED PHASES OF EVOLUTION OF POPULATION 2 STARS - GROWTH OF CARBON CORE AND SHELL HELIUM FLASHES
HAYASHI, C
HOSHI, R
SUGIMOTO, D
[J]. PROGRESS OF THEORETICAL PHYSICS, 1965, 34 (06): : 885 - &
[7] HAYASHI C, 1962, PROG THEOR PHYS S22, P1
[8] THERMAL INSTABILITY IN A NUCLEAR-BURNING SHELL OF STARS
HOSHI, R
[J]. PROGRESS OF THEORETICAL PHYSICS, 1968, 39 (04): : 957 - &
[9] STELLAR EVOLUTION TOWARD PRE-SUPERNOVA STAGE .1. CARBON AND OXYGEN STARS OF 5M, 10M AND 30M
IKEUCHI, S
NAKAZAWA, K
HAYASHI, C
HOSHI, R
MURAI, T
[J]. PROGRESS OF THEORETICAL PHYSICS, 1971, 46 (06): : 1713 - &
[10] EVOLUTION OF INITIALLY PURE 12C STARS AND PRODUCTION OF PLANETARY NEBULAE
KUTTER, GS
SAVEDOFF, MP
[J]. ASTROPHYSICAL JOURNAL, 1969, 156 (3P1) : 1021 - &