Hydrogen Flux in the Semiconvection Zone of the Massive Main Sequence Stars

Details Hydrogen Flux in the Semiconvection Zone of the Massive Main Sequence Stars Hydrogen Flux in the Semiconvection Zone of the Massive Main Sequence Stars

Sep 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998ap%26ss.259..343u&link_type=abstract

Astrophysics and Space Science, v. 259, Issue 4, p. 343-354 (1998).

Astronomy and Astrophysics

Astrophysics

3

Scientific paper

We find that the hydrogen flux near the boundary of the semiconvection
zone with Ledoux's neutral condition is unreasonably positive while it
is reasonably negative throughout the semiconvection zone with
Schwarzschild's neutral condition.

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