The ratio of small to large separations of stellar p-modes
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK e-mail: firstname.lastname@example.org
2 LESIA, Observatoire de Paris, Place Jules Janssen, 92195 Meudon, France
Accepted: 23 December 2004
In previous papers we showed that the ratios of the small to large separations of acoustic oscillations in solar-like stars are approximately independent of the structure of the outer layers, and are therefore diagnostics of the interior structure alone. Here we present similar results for a range stellar models of mass , all of which show this same property.
Key words: stars: oscillations / stars: interiors
© ESO, 2005