All Tables
- Table 10:
Spectroscopic
and Li abundances1 derived for the
subgroup of Li detected (left) and Li non-detected stars (right).
- Table 11:
Sensitivity of the derived Li abundances (in dex) to slight
changes in the model atmosphere parameters for IRAS 15255+1944.
- Table 12:
Distribution of sources among the different subgroups identified in
the sample as a function of their OH expansion velocity and variability
properties.
- Table 1:
The sample of Galactic O-rich AGB stars.
- Table 2:
The sample of comparison stars.
- Table 3:
The sample of peculiar carbon AGB stars.
- Table 4:
Log of the spectroscopic observations.
- Table 5:
Galactic O-rich AGB stars where the lithium line was detected.
- Table 6:
Galactic O-rich AGB stars where the lithium line was not detected.
- Table 7:
Galactic O-rich AGB stars for which no analysis of the lithium line was possible.
- Table 8:
Comparison stars.
- Table 9:
Peculiar C-rich AGB stars.