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Table 1
Masers detected toward G345.5+1.5.
| ℓ | b | Masers | Velocity | Kinematic distance | References |
|---|---|---|---|---|---|
| (°) | (km s−1) | (kpc) | |||
| 345.013 | 1.798 | 1.665 GHz-OH | −23 | 2.5 | Caswell & Haynes (1983); Caswell et al. (1995a) |
| 22 GHz-H2O | −18 | 2.1 | Caswell et al. (1983); Forster & Caswell (1989) | ||
| 12 GHz-CH3OH | −17 | 2.0 | Caswell & Haynes (1983); Caswell et al. (1995b) | ||
| 6.6 GHz-CH3OH | −18 | 2.1 | Menten (1991); Caswell et al. (1995a) | ||
| 6.035 GHz-OH | −20 | 2.3 | Caswell & Vaile (1995) | ||
| 4.7 GHz-OH | −25 | 2.7 | Cohen et al. (1995) | ||
| 345.015 | 1.801 | 22 GHz-H2O | −20 | 2.3 | Caswell et al. (1983) |
| 6.6 GHz-CH3OH | −13 | 1.6 | Caswell et al. (1995c,a) | ||
| 12 GHz-CH3OH | −13 | 1.6 | Caswell et al. (1995b,c) | ||
| 345.123 | 1.592 | 1.7 GHz-OH | −17 | 2.0 | Caswell (2004) |
| 345.464 | 1.460 | 4.7 GHz-OH | −15 | 1.9 | Cohen et al. (1995) |
| 345.492 | 1.470 | 4.7 GHz-OH | −15 | 1.9 | Cohen et al. (1995) |
| 1.7 GHz-OH | −15 | 1.9 | Caswell (2004) | ||
| 345.210 | 1.035 | 4.7 GHz-OH | −9 | 1.2 | Cohen et al. (1995) |
Notes. Thekinematic distance is computed following the model of Reid et al. (2014), which can be found at http://bessel.vlbi-astrometry.org/revised_kd_2014
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