Jun 1988
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988sci...240.1743w&link_type=abstract
Science (ISSN 0036-8075), vol. 240, June 24, 1988, p. 1743-1750.
Physics
11
Mixing, Nuclear Reactions, Stellar Atmospheres, Stellar Interiors, Stellar Physics, Carbon Stars, Convection, Main Sequence Stars, Mass Transfer, S Stars, Stellar Composition, Stellar Spectra, Stellar Structure, Time Measurement
Scientific paper
Analysis of the chemical and isotopic composition of stellar surfaces reveals the types of nuclear reactions that have occurred in the stellar interiors as well as the timing and depths from which material once deep in the star has reached the surface. Mass loss from the stellar surface and, in some cases, mass transfer from a companion enhance the opportunity to observe material that is the product of internal nuclear reactions. Detailed studies show substantial deficiencies in current models with the timing and depth of convective and other forms of mixing.
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