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Deep Circulation in Red Giant Stars: A Solution to the Carbon and Oxygen
Isotope Puzzles?
G. J. Wasserburg (Caltech),
Arnold I. Boothroyd (CITA), and
I.-Juliana Sackmann (Caltech)
Astrophysical Journal (Letters),
447, L37-L40 (1995)
Available as:
-
PDF (205 kb: 11 pages, including figs);
or
- gzip'd
PostScript (129 kb, expands to 498 kb: 11 pages, including figs);
or
-
gzip'd tar-file archive (88 kb, expands to 317 kb), including
plain TeX text (47 kb: 6 pages) and 4 Postscript figures.
See also the more comprehensive discussion in
our CNO paper of 1999. It looks like the oxygen puzzle may not
be solved by deep circulation and cool bottom processing.
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