On the pulsation mode of Mira variables: Nonlinear calculations compared with radii observations

被引：17

作者：

Ya'ari, A ^{[1
]}

Tuchman, Y ^{[1
]}

机构：

[1] Hebrew Univ Jerusalem, Racah Inst Phys, IL-91904 Jerusalem, Israel

来源：

ASTROPHYSICAL JOURNAL | 1999年 / 514卷 / 01期

关键词：

stars : fundamental parameters; stars : late-type; stars : oscillations;

D O I：

10.1086/311932

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Observed radii of Mira variables are compared with theoretical nonlinear calculations. In contrast with previous works, the observed data is found to be compatible with the fundamental nonlinear mode of pulsation.

引用

页码：L35 / L37

页数：3

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