All Tables

• Table 1: Results of single Gaussian (top) and 7-component HFS (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.