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BIBTEX RIS

The fundamental parameters of the roAp star HD 24712

2016; EDP Sciences; Volume: 590; Linguagem: Inglês

10.1051/0004-6361/201527920

ISSN

1432-0746

Autores

K. Perraut, I. M. Brandão, M. S. Cunha, D. Shulyak, D. Mourard, N. Nardetto, Theo A. ten Brummelaar,

Tópico(s)

Astrophysics and Star Formation Studies

Resumo

Context. There is still a debate about the nature of the mechanism that causes the pulsation excitation of the rapidly oscillating Ap stars that oscillate above the highest theoretically acoustic frequency. HD 24712 is a good test case for such a study because it is bright, its parallax accurately determined, and its frequency spectrum is well known.

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