Modelling spectro-photometric characteristics of nonradially pulsating stars

被引：0

作者：

Daszynska, J ^{[1
]}

Cugier, H ^{[1
]}

机构：

[1] Univ Wroclaw, Astron Inst, PL-51622 Wroclaw, Poland

来源：

ASTRONOMICAL DATA ANALYSIS SOFTWARE AND SYSTEMS VII (ADASS) | 1998年 / 145卷

关键词：

D O I：

暂无

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

We present a computing code for modelling energy flux distributions, photometric indices and spectral line profiles of (non-)radially pulsating Main-Sequence stars. The model is based on the perturbation-expansion formalism taking into account geometrical and nonadiabatic effects.

引用

页码：11 / 14

页数：4