Physics
Scientific paper
Dec 2008
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2008phst..133a4029e&link_type=abstract
Physica Scripta, Volume 133, Issue , pp. 014029 (2008).
Physics
Scientific paper
A brief progress report is given on an on-going project to estimate the
C, N and O abundances in carbon stars of the Magellanic Cloud clusters
NGC 1846 and NGC 419. The changes in these abundances as a function of
position along the asymptotic giant branch (AGB) are sought for.
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