The ratio of small to large separations of stellar p-modes
Résumé
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 0.8, 1.0, 1.2, 1.5, 2, 10~ M_&sun;, all of which show this same property.
Domaines
Astrophysique [astro-ph]
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