High mass loss in the young Sun

Details High mass loss in the young Sun High mass loss in the young Sun

Dec 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988esasp.286..629t&link_type=abstract

In ESA, Seismology of the Sun and Sun-Like Stars p 629-635 (SEE N89-25819 19-92)

Physics

3

Stellar Mass Ejection, Stellar Models, Stellar Physics, Sun, Abundance, Solar Oscillations, Stellar Composition, Stellar Evolution

Scientific paper

The consequences of a possible mass loss in the early main sequence stage of solar type stars are investigated. Special attention is given to the Sun; the constraints from surface abundances and p-mode observations are taken into account. Only a total mass loss smaller than 0.2 solar M seems to be consistent with the observations. Though the ensuing modifications of the internal structure and the cosmological consequences are very small, the He3, Li7, Be9 surface abundances are significantly modified.

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