Table 1
6.7 GHz methanol masers observed at multiple wavelengths to determine SEDs.
Source | α | δ | S p | d | L m |
(J2000) | (J2000) | (Jy) | (kpc) | (L⊙) | |
|
|||||
38.66+0.08 | 19 01 35.24 | 05 07 47.4 | 0.71 | 16.3 ± 0.9 | (1.3 ± 0.2) × 10-6 |
38.92–0.36 | 19 03 38.66 | 05 09 42.5 | 1.29 | 10.5 ± 0.4 | (9.9 ± 0.8) × 10-7 |
39.39–0.14 | 19 03 45.32 | 05 40 42.6 | 0.77 | 4.3 ± 0.5 | (9.9 ± 2.3) × 10-8 |
39.54–0.38 | 19 04 52.6 | 05 42 08 | 0.24 | 9.0 ± 0.5 | (1.3 ± 0.2) × 10-7 |
40.28–0.22 | 19 05 41.22 | 06 26 12.7 | 68.03 |
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40.62–0.14 | 19 06 01.59 | 06 46 36.1 | 6.97 | 10.5 ± 0.4 | (5.3 ± 0.4) × 10-6 |
40.94–0.04 | 19 06 15.38 | 07 05 54.5 | 1.50 | 10.0 ± 0.5 | (1.0 ± 0.1) × 10-6 |
41.08–0.13a | 19 06 48.5 | 07 11 00 | 0.33 | 8.4 ± 0.6 | (1.6 ± 0.3) × 10-7 |
41.12–0.11 | 19 06 50.2 | 07 14 02 | 0.63 | 10.0 ± 0.5 | (4.4 ± 0.5) × 10-7 |
41.12–0.22 | 19 07 14.86 | 07 11 00.7 | 1.23 | 8.7 ± 0.6 | (6.5 ± 0.9) × 10-7 |
41.16–0.20 | 19 07 14.3 | 07 13 19 | 0.20 | 8.7 ± 0.6 | (1.0 ± 0.2) × 10-7 |
41.23–0.20 | 19 07 21.38 | 07 17 08.2 | 7.55 | 8.7 ± 0.5 | (4.0 ± 0.5) × 10-6 |
41.27+0.37 | 19 05 23.6 | 07 35 06 | 0.16 | 11.5 ± 0.5 | (1.5 ± 0.2) × 10-7 |
41.34–0.14 | 19 07 21.84 | 07 25 17.3 | 25.40 | 11.6 ± 0.5 | (2.4 ± 0.2) × 10-5 |
41.58+0.04 | 19 07 09.1 | 07 42 25 | 0.22 | 11.5 ± 0.5 | (2.0 ± 0.2) × 10-7 |
42.03+0.19 | 19 07 28.18 | 08 10 53.5 | 30.10 | 11.1 ± 0.5 | (2.6 ± 0.3) × 10-5 |
42.30–0.30 | 19 09 43.59 | 08 11 41.4 | 5.07 | 10.5 ± 0.5 | (3.9 ± 0.4) × 10-6 |
42.43–0.26 | 19 09 49.86 | 08 19 45.4 | 1.61 | 7.9 ± 0.8 | (7.0 ± 1.4) × 10-7 |
42.70–0.15 | 19 09 55.07 | 08 36 53.5 | 4.03 | 15.9 ± 0.8 | (7.1 ± 0.7) × 10-6 |
43.08–0.08 | 19 10 22.05 | 08 58 51.5 | 4.11 | 11.2 ± 0.5 | (3.6 ± 0.3) × 10-6 |
Notes. The columns show the source name, equatorial J2000 coordinates, peak flux density, distance and luminosity. Positions that are accurate to 0.1'' are derived from MERLIN observations, while positions accurate to 1'' are derived from MIPSGAL 24 μm point sources.
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