Mass limits for non-degenerate white dwarfs

Details Mass limits for non-degenerate white dwarfs Mass limits for non-degenerate white dwarfs

Jul 1981

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1981nupha.364..527s&link_type=abstract

Nuclear Physics A, Volume 364, Issue 2-3, p. 527-532.

Physics

Nuclear Physics

1

Scientific paper

We obtain the dependence of the upper mass limit of white dwarf stars on
the specific entropy per electron. For non-degenerate stars
significantly larger masses are found. Stellar collapse as an
entropy-producing process can therefore have a self-stabilizing
influence on the stellar evolution.

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