Physics
Scientific paper
Oct 1992
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1992s%26w....31..616l&link_type=abstract
Sterne und Weltraum (ISSN 0039-1263), vol. 31, no. 10, p. 616-621.
Physics
Stellar Convection, Stellar Evolution, Stellar Interiors, Stellar Physics, Supernova 1987A, Massive Stars, Mixing, Stellar Models
Scientific paper
Theoretical models are used here to examine the interior of stars and
the role of mixing processes there. The effect of those processes on the
development of massive stars and in particular on the blue color of the
SN 1987A progenitor is addressed.
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