Hydrodynamical instabilities in the envelopes of main-sequence stars - Constraints implied by the lithium, beryllium, and boron observations

Details Hydrodynamical instabilities in the envelopes of main-sequence stars - Constraints implied by the lithium, beryllium, and boron observations Hydrodynamical instabilities in the envelopes of main-sequence stars - Constraints implied by the lithium, beryllium, and boron observations

Jul 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978apj...223..567v&link_type=abstract

Astrophysical Journal, Part 1, vol. 223, July 15, 1978, p. 567-582.

Astronomy and Astrophysics

Astrophysics

84

Abundance, Magnetohydrodynamic Stability, Main Sequence Stars, Stellar Envelopes, Beryllium, Boron, Convective Flow, Laminar Flow, Lithium, Meridional Flow

Scientific paper

Abstract image available at:
http://adsabs.harvard.edu/abs/1978ApJ...223..567V

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