NORMAL MODES OF RADIAL PULSATION OF STARS AT END POINT OF THERMONUCLEAR EVOLUTION

被引：118

作者：

MELTZER, DW

THORNE, KS

机构：

来源：

关键词：

D O I：

10.1086/148792

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

引用

页码：514 / +

页数：1

共 45 条

[11] CHIU HY, 1964, GRAVITATION RELATIVI, pCH10
[12] VIBRATIONAL ENERGY OF NEUTRON STARS AND EXPONENTIAL LIGHT CURVES OF TYPE-I SUPERNOVAE
FINZI, A
[J]. PHYSICAL REVIEW LETTERS, 1965, 15 (15) : 599 - &
[13] COOLING OF A NEUTRON STAR BY URCA PROCESS
FINZI, A
[J]. PHYSICAL REVIEW, 1965, 137 (2B): : B472 - &
[14] GOLDBERG L, 1966, ANNUAL REVIEWS AS ED, V4
[15] MODELS FOR ZERO-TEMPERATURE STARS
HAMADA, T
SALPETER, EE
[J]. ASTROPHYSICAL JOURNAL, 1961, 134 (03) : 683 - 698
[16] ASYMPTOTIC BEHAVIOR OF COLD SUPERDENSE STARS
HARRISON, BK
[J]. PHYSICAL REVIEW, 1965, 137 (6B): : 1644 - &
[17] HARRISON BK, IN PREPARATION
[18] HARRISON BK, 1965, GRAVIATION THEORY GR
[19] HARRISON BK, 1958, 11 CONS PHYS SOLV
[20] ELECTROMAGNETIC WAVES FROM VERY DENSE STARS
HOYLE, F
WHEELER, JA
NARLIKAR, JV
[J]. NATURE, 1964, 203 (494) : 914 - +