Table A.5.
Observational results for those sources which clearly show double-component in the 12CO J = 2 − 1 line (type 4 profiles).
| Source | Components | A | Tmb | Vlsr | Vexp |
|---|---|---|---|---|---|
| (K km s−1) | (K) | (km s−1) | (km s−1) | ||
| V370 And | Broad | 35.87 | 2.51 | −1.94 | 10.97 |
| Narrow | 13.93 | 5.65 | −2.03 | 3.03 | |
| X Her | Broad | 29.89 | 2.16 | −73.46 | 9.46 |
| Narrow | 13.15 | 5.51 | −73.01 | 2.94 | |
| EP Aqr | Broad | 51.70 | 3.18 | −33.95 | 11.51 |
| Narrow | 12.37 | 9.85 | −33.41 | 2.05 | |
| IQ Aqr | Broad | 1.20 | 0.06 | 21.24 | 12.48 |
| Narrow | 2.07 | 0.33 | 20.71 | 6.02 |
Notes. Description of the columns from left to right: (1) GCVS designation (Samus et al. 2009); (2) component; (3–6) integrated line intensity, peak main-beam brightness temperature, systemic velocity, and expansion velocity for each component. We note that the peak main-beam brightness temperature of the narrow components coincides with the peak main-beam brightness temperature of the entire emission lines (see Table A.1). For the integrated line intensity, the situation is more complex (see text).
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