| Issue |
A&A
Volume 434, Number 2, May I 2005
|
|
|---|---|---|
| Page(s) | 665 - 669 | |
| Section | Stellar structure and evolution | |
| DOI | https://doi.org/10.1051/0004-6361:20041957 | |
| Published online | 11 April 2005 | |
The ratio of small to large separations of stellar p-modes
1
Astronomy Unit, Queen Mary, University of London, Mile End Road, London E1 4NS, UK e-mail: i.w.roxburgh@qmul.ac.uk
2
LESIA, Observatoire de Paris, Place Jules Janssen, 92195 Meudon, France
Received:
6
September
2004
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
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