On nonradial thermal instability in stars

Details On nonradial thermal instability in stars On nonradial thermal instability in stars

Jun 1979

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1979pazh....5..242v&link_type=abstract

(Pis'ma v Astronomicheskii Zhurnal, vol. 5, May 1979, p. 242-245.) Soviet Astronomy Letters, vol. 5, May-June 1979, p. 128-130.

Astronomy and Astrophysics

Astrophysics

1

Astrophysics, Atmospheric Circulation, Early Stars, Stellar Models, Thermal Instability, Abundance, Carbon, Chemical Composition, Nitrogen, Oxygen, Self Excitation, Stellar Evolution

Scientific paper

Circulation can be self-excited within a convectively stable zone in
which energy is produced by the CNO cycle. The self-excitation would be
facilitated by a heavy-element abundance increasing with depth. The
development of such thermal instability could result in a stellar energy
source asymmetric in both chemical composition and temperature.

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