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Table B.5
H2O maser emission (our VLA observations) and OH (from the literature) maser emission of IRAS 18480+0008.
| Maser coordinates | δR.A. | δdec | Transition | VLSR | Sν | |
|---|---|---|---|---|---|---|
| R.A.(J2000) | Dec(J2000) | (arsec) | (arsec) | (MHz) | (km s−1) | (Jy) |
| 18:50:36.685 | +00:12:28.34 | 0.10 | 0.10 | 1665 | +12.00 | 0.345±0.009 |
| 18:50:36.66107 | +00:12:28.140 | 0.0009 | 0.020 | 22235 | +14.53 | 1.026±0.011 |
| 18:50:36.6635 | +00:12:28.21 | 0.003 | 0.05 | 22235 | +18.75 | 0.244±0.007 |
| 18:50:36.6720 | +00:12:28.41 | 0.017 | 0.17 | 22235 | +20.22 | 0.110±0.012 |
| 18:50:36.66141 | +00:12:28.191 | 0.0004 | 0.007 | 22235 | +22.54 | 1.9844±0.0008 |
| 18:50:36.66040 | +00:12:28.07 | 0.0013 | 0.03 | 22235 | +25.07 | 0.690±0.010 |
| 18:50:36.66330 | +00:12:28.147 | 0.0010 | 0.020 | 22235 | +26.54 | 0.782±0.009 |
Notes. The parameters of the OH maser transition at 1665 MHz were reported by Beuther et al. (2019).
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