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BIBTEX RIS

A spectroscopic study of southern (candidate) γ Doradus stars

2007; EDP Sciences; Volume: 478; Issue: 2 Linguagem: Inglês

10.1051/0004-6361

ISSN

1432-0746

Autores

H. Bruntt, P. De Cat, C. Aerts,

Tópico(s)

Astro and Planetary Science

Resumo

Context.The γ Doradus stars are a recent class of variable main sequence F-type stars located on the red edge of the Cepheid instability strip. They pulsate in gravity modes, and this makes them particularly interesting for detailed asteroseismic analysis, which can provide fundamental knowledge of properties near the convective cores of intermediate-mass main sequence stars.

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