Table 5
Results for the inner-GB sources.
| Source | SED type | P(a) (days) | L(b) (L⊙) |  (c) (M⊙ yr−1) |
Rgd(d) | vsys(e) (km s−1) | v∞(e) (km s−1) | 12CO/13CO(f) |
|---|---|---|---|---|---|---|---|---|
| 1 - OH358.083+0.137 | DE | np | 2100 | 2 × 10−5 | 29 | −24 | 22 | 5 |
| 4 - OH358.505+0.330 | DE | np | 6500 | 1 × 10−4 | 125 | −30 | 24 | 5 |
| 5 - OH359.140+1.137 | DE | 1000 | 6100 | 1 × 10−5 | 8 | −136 | 12 | 3 |
| 7 - OH359.220+0.163 | DE | np | 3400 | 8 × 10−5 | 67 | −137 | 16 | 7 |
| 8 - OH359.233−1.876 | DE | np | 3400 | 3 × 10−5 | 20 | −15 | 18 | 4 |
| 9 - OH359.467+1.029 | SE | 605 | 5600 | 2 × 10−5 | 200 | 110 | 18 | 13 |
| 10 - OH359.543−1.775 | DE | mp | 5400 | 2 × 10−5 | 12 | 90 | 36 | 2 |
| 11 - OH359.664+0.636 | SE | 550 | 6100 | 2 × 10−5 | 250 | −158 | 13 | 5 |
| 12 - OH359.745−0.404 | SE | 730 | 6000 | 1 × 10−5 | 100 | 186 | 21 | 2 |
| 13 - OH359.805+0.200(g) | SE | 500 | 4300 | 5 × 10−6 | 71 | −51 | 21 | 4 |
| 14 - OH359.826+0.153 | SE | 500 | 5600 | 6 × 10−6 | 171 | −26 | 17 | 7 |
| 15 - OH359.902+0.061 | SE | 590 | 4300 | 1 × 10−5 | 250 | −133 | 19 | 4 |
| 16 - OH0.173+0.211(g) | SE | 512 | 3300 | 1 × 10−5 | 333 | 52 | 18 | |
| 17 - OH0.221+0.168 | SE | 663 | 5300 | 1 × 10−5 | 200 | 64 | 23 | 10 |
| 19 - OH0.739+0.411 | SE | 570 | 25000 | 3 × 10−5 | 176 | −21 | 12 | 8 |
| 21 - OH1.221+0.294 | SE | 715 | 8700 | 7 × 10−5 | 778 | −261 | 13 | 50 |
| 22 - OH1.628+0.617 | SE | 830 | 25000 | 5 × 10−5 | 250 | −86 | 27 | 16 |
Notes. (a) The adopted period from Table 3 (np = non-periodic, mp = non-Mira multi-periodic variablity).(b) Obtained by integrating the fit to the extinction-corrected SEDs.(c) The uncertainty is estimated to be a factor of 5.(d) The gas-to-dust mass ratio estimated as 
. The uncertainty is estimated to be a factor of seven. (e) Estimated as weighted averages of the results for the detected CO lines. The uncertainties are estimated to be ± 1.0 and ± 1.5 km s−1 for the systemic and expansion velocities, respectively.(f) The uncertainty is estimated to be a factor of 4.(g) Only the 12CO(J = 2–1) line is used for the mass-loss-rate estimate.
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