Evolution, Structure, and Seismology of Intermediate-Mass Stars

Details Evolution, Structure, and Seismology of Intermediate-Mass Stars Evolution, Structure, and Seismology of Intermediate-Mass Stars

Apr 2002

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2002apj...569..911g&link_type=abstract

The Astrophysical Journal, Volume 569, Issue 2, pp. 911-940.

Astronomy and Astrophysics

Astronomy

7

Stars: Evolution, Stars: Interiors, Stars: Oscillations

Scientific paper

The interior structure, the evolution, and the p-mode oscillation spectra of stellar models between 2.0 and 5 Msolar are presented. Interior details, including convective core and envelope growth and decay, the development of composition gradients, and the onset of hydrogen shell burning are shown to be testable by future asteroseismology observations. The stellar age and mass dependence of the large- and small-spacing oscillation frequencies are discussed. The dependencies of the structure and the oscillation spectra on composition and mixing length are also discussed. A new oscillation diagnostic for stellar mass is introduced.

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