Table 3.
Detected line properties.
| Source | Line | υcen | Speak | FWHM | Sint | Lline |
|---|---|---|---|---|---|---|
| [km s−1] | [mJy] | [km s−1] | [Jy km s−1] | [×108 L⊙] | ||
| W0149+2350 | H2O(202 − 111) | |||||
| comp1 | −219 ± 103 | 1.3 ± 0.2 | 564 ± 413 | 0.80 ± 0.60 | 1.58 ± 1.17 | |
| comp2 | 396 ± 58 | 1.4 ± 0.2 | 421 ± 99 | 0.63 ± 0.18 | 1.24 ± 0.36 | |
| Total | > 1.12 | > 2.2 | ||||
| W0410−0913 | H2O(312 − 303) | |||||
| comp1 | −307 ± 44 | 1.2 ± 0.7 | 256 ± 167 | 0.31 ± 0.29 | 0.83 ± 0.76 | |
| comp2 | 99 ± 54 | 3.8 ± 0.2 | 737 ± 103 | 2.99 ± 0.46 | 7.90 ± 1.23 | |
| Total | 3.30 ± 0.54 | 8.73 ± 1.44 | ||||
| OH+(11 − 01) | −100 ± 83 | 2.6 ± 0.3 | 1000 ± 196 | 2.78 ± 0.62 | 6.92 ± 1.55 | |
Notes. For each emission line we give the central velocity (υcen), peak flux (Speak), FWHM, and integrated flux (Sint), based on the Gaussian fits to the line. The corresponding line luminosity (Lline) is also given. The H2O emission for both sources is best fit by a double Gaussian, therefore the parameters of the two components corresponding to the fit are listed. In the case of W0149+2350, where the line is truncated, a lower limit is given on the total Sint and Lline based on the integration of the observed spectral line.
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