An observational approach to convection in main sequence stars

Bibcode
2005A&A...443.1013R
DOI
10.1051/0004-6361:20053620
Régulo, C.; Vázquez Ramió, H.; Roca Cortés, T.
Referencia bibliográfica

Astronomy and Astrophysics, Volume 443, Issue 3, December I 2005, pp.1013-1019

Fecha de publicación:
12
2005
Revista
Astronomy and Astrophysics
Número de autores
3
Número de autores del IAC
3
Número de citas
2
Número de citas referidas
2
Descripción
Observational results concerning possible changes in the granulation of Main Sequence stars were found by analysing their seismic power spectra obtained from photometric microvariability. We analysed as many as 178 stars with spectral types F, G, K, and M observed for 54 days. We present evidence of changes in the lifetime and contrast of the granulation, which both increase from F to M stars, although within the limit of resolution.
Tipo
Con árbitro

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