Mixing in close binaries

Details Mixing in close binaries Mixing in close binaries

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989pazh...15.1008l&link_type=abstract

Pis'ma v Astronomicheskii Zhurnal (ISSN 0320-0108), vol. 15, Nov. 1989, p. 1008-1015. In Russian. In Russian. In Russian.

Physics

2

Binary Stars, Stellar Composition, Stellar Physics, Carbon, Helium, Mixing, Nitrogen, Thermonuclear Reactions

Scientific paper

Consideration is given to mixing of matter in radiative zones of main-sequence stars which enter close synchronized binary systems. The mixing is created by slow circulation currents which maintain the thermal balance and may be responsible for the excesses of N-14 and H-4 and the deficit of C-12 observed in the surface layers of close binary components.

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