RADIAL OSCILLATION PERIODS FOR HAMADA-SALPETER MODELS OF WHITE DWARFS

被引：8

作者：

SKILLING, J

机构：

[1] Mullard Radio Astronomy Observatory, Cavendish Laboratory

来源：

NATURE | 1968年 / 218卷 / 5141期

关键词：

D O I：

10.1038/218531b0

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Calculations of the oscillation periods for white dwarf models show that, until instability is reached, the period depends very little on the composition or the equation of state © 1968 Nature Publishing Group.

引用

页码：531 / &

共 5 条

[1] MODELS FOR ZERO-TEMPERATURE STARS [J].

HAMADA, T ;

SALPETER, EE .

ASTROPHYSICAL JOURNAL, 1961, 134 (03) :683-698

[2] OBSERVATION OF A RAPIDLY PULSATING RADIO SOURCE [J].

HEWISH, A ;

BELL, SJ ;

PILKINGT.JD ;

SCOTT, PF ;

COLLINS, RA .

NATURE, 1968, 217 (5130) :709-&

[3]

LEDOUX P, 1958, HANDBUCH PHYSIK, V51, P463

[4] NORMAL MODES OF RADIAL PULSATION OF STARS AT END POINT OF THERMONUCLEAR EVOLUTION [J].

MELTZER, DW ;

THORNE, KS .

ASTROPHYSICAL JOURNAL, 1966, 145 (02) :514-+

[5] ENERGY AND PRESSURE OF A ZERO-TEMPERATURE PLASMA [J].

SALPETER, EE .

ASTROPHYSICAL JOURNAL, 1961, 134 (03) :669-682

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