Astronomy and Astrophysics – Astrophysics
Scientific paper
Feb 1986
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986a%26a...156..391b&link_type=abstract
Astronomy and Astrophysics (ISSN 0004-6361), vol. 156, no. 1-2, Feb. 1986, p. 391, 392.
Astronomy and Astrophysics
Astrophysics
4
Dwarf Stars, Polytropic Processes, Red Giant Stars, Stellar Evolution, Molecular Weight, Stellar Cores, Stellar Envelopes, Stellar Gravitation
Scientific paper
The author considers the processes that may explain why dwarf stars become red giants after they complete central hydrogen burning. It seems clear that it is the development of a molecular weight gradient and an increased gravitational field at the central core boundary that conspire to transform a star into a red giant. The author indicates here that both of these effects can have an explanation in terms of simple polytropes; nuclear evolution and the change to shell hydrogen burning both act in the sense of increasing the star averaged polytropic index >n< towards its maximum value of five.
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