- Table 1:
Parameter space used for the models and the astrophysical parameters
of the standard star Vega and the Bootis stars HD 107233 and HD 204041.
- Table 2:
Location of the stars according to Fig. 1.
The results for the individual stars are listed in Table 3.
- Table 3:
The results for
Bootis stars taken from Paunzen et al. (2002)
according to Fig. 1 and Table 2.
We would only consider the stars of group (5)
as good candidates for undetected spectroscopic binary systems, and
no conclusion can be drawn for group (6).