Stellar initial-final mass relations.

Details Stellar initial-final mass relations. Stellar initial-final mass relations.

Oct 1997

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1997acaps..17..393h&link_type=abstract

Acta Astrophys. Sin., Vol. 17, No. 4, p. 393 - 400

Astronomy and Astrophysics

Astrophysics

Agb Stars: Masses, Stellar Evolution: Mass Loss, Population I Stars: Masses, Population Ii Stars: Masses, Planetary Nebulae: Nuclei

Scientific paper

The author studied the relationship between the zero-age mass of a Pop I star and the mass of its degenerate core at the point in the star's evolution when the binding energy of its envelope changes from negative to positive. The relation is found to be consistent with the initial-final mass relation of Weidemann and Koester, and also agrees with the distribution of masses of planetary nebula nuclei observed by Zhang and Kwok. A similar relation is obtained for Pop II stars.

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