The ratio of small to large separations of stellar p-modes

Details The ratio of small to large separations of stellar p-modes The ratio of small to large separations of stellar p-modes

May 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005a%26a...434..665r&link_type=abstract

Astronomy and Astrophysics, Volume 434, Issue 2, May I 2005, pp.665-669

Astronomy and Astrophysics

Astrophysics

24

Stars: Oscillations, Stars: Interiors

Scientific paper

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.

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