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What can we expect from precision asteroseismology?

Published online by Cambridge University Press:  18 February 2014

G. Handler
G. Handler*
Affiliation:
Nicolaus Copernicus Astronomical Center, Bartycka 18, 00-716 Warsaw, Poland email: gerald@camk.edu.pl
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Abstract

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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.

Keywords

stars: abundancesstars: atmospheresstars: early-typestars: fundamental parametersstars: interiorsstars: late-typestars: oscillationsconvectiondiffusionatomic data
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S301: Precision Asteroseismology , August 2013 , pp. 23 - 26
Copyright
Copyright © International Astronomical Union 2014 

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