What can we expect from precision asteroseismology?

被引：0

作者：

Handler, G. ^{[1
]}

机构：

[1] Nicolaus Copernicus Astron Ctr, Bartycka 18, PL-00716 Warsaw, Poland

来源：

PRECISION ASTEROSEISMOLOGY | 2014年 / 9卷 / 301期

关键词：

stars: abundances; stars: atmospheres; stars: early-type; stars: fundamental parameters; stars: interiors; stars: late-type; stars: oscillations; convection; diffusion; atomic data; STAR; INSTABILITIES; HYDROGEN; ROTATION;

D O I：

10.1017/S1743921313014014

中图分类号：

P1 [天文学];

学科分类号：

0704 ;

摘要：

Precision asteroseismology is the determination of accurate stellar parameters from oscillation data. At first successful for pulsating white dwarf stars, it is now applied to more and more types of stars. We give a number of selected examples where precision asteroseismology, but also asteroseismology based on few observables may lead to considerable improvement of stellar astrophysics in the near future.

引用

页码：23 / 26

页数：4

共 25 条

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