- Table 1:
Results of single Gaussian (top) and 7-component
(bottom) fits to the spectra observed toward the center of Cha-MMS1.
- Table 2:
Gas temperature, non-thermal broadening and abundance of each
molecule for the best-fit model. The peak opacity of each modeled transition
is also given, as well as an estimation of the total opacity of the hyperfine
multiplets if they had been modeled.