Radial vibrations in a 5 solar M hydrogen-helium star

Details Radial vibrations in a 5 solar M hydrogen-helium star Radial vibrations in a 5 solar M hydrogen-helium star

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..657k&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 657-660 (SEE N89-25819 19-92)

Physics

B Stars, Stellar Evolution, Stellar Luminosity, Stellar Models, Stellar Physics, Adiabatic Conditions, Pulses, Stellar Composition, Stellar Oscillations

Scientific paper

A model of a first-generation intermediate mass star with no metals is
considered. The vibrational instability of this model is investigated.
The model burns helium in the core. Calculations were performed for the
first and second harmonics as well as for the fundamental mode. The
model is found to be vibrationally stable toward radial pulsations.

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