Journal
ASTRONOMY & ASTROPHYSICS
Volume 434, Issue 2, Pages 665-669Publisher
E D P SCIENCES
DOI: 10.1051/0004-6361:20041957
Keywords
stars : oscillations; stars : interiors
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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 ., all of which show this same property.
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