All Tables
- Table 1:
Mass and radius determination for
CMa from the Harmanec (1988) compilation for the effective temperatures given by Popper (1980), Prinja (1989) and Fremat (2005).
- Table 2:
Calibration star diameters estimated from spectro-photometric
indices (computed as in Bonneau et al. 2006)
and their associated errors.
- Table 3:
Br
visibilities measured in the continuum (
)
and visibility drop within the Br
line
(
/
).
calculated from the measured
and
/
ratio. The deduced envelope contribution in the
continuum (
)
and in the line (
)
is given for each
baseline. The corresponding angular diameters in the Br
line (
)
and the nearby continuum (
)
are
computed using a uniform disk model for each envelope
measurement. The corresponding extension in stellar radii are
also given, assuming a 6
star at 230 pc.
- Table 4:
Parameters for the
CMa central star and its
circumstellar environment for the best axi-symetric model.