All Tables
- Table 1:
Measured circumstellar ratios, and simulated emission
intensities for the transitions under consideration. The circumstellar
factors are taken from calibrated ESO/HARPS spectra of
Pic (Galland F., Priv. Comm.). The emission intensities (given
in arbitrary units) out of the mid-plane are derived from the
CLOUDY run and those in the midplane are estimated by
multiplying the former ones by the circumstellar factors.
- Table 2:
Values of the critical impact parameter b0 as a function
of the relative velocity v, as computed from Eq. (6) for the Ca II-H I interaction.