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Table 1

Target sources and observed species.

Source α δ vlsr Obs. species OD Type
(J2000) (J2000) (km s−1) detection
G10.47+0.03 18:08:38.20 −19:51:50.0 +66.8(a) OD, OH abs UCHII, hot core(1,2,3)
G23.21−0.3 18:34:54.91 − 08:49:19.2 + 76.8(a) OD abs quiescent
G34.26+0.15 18:53:18.49 01:14:58.7 +58.1(a) OD, OH, 18OH abs UCHII, hot core(1,3)
G34.41+0.2 18:53:18.13 01:25:23.7 + 57.6(a) OD Quiescent
G35.20−0.7 18:58:12.93 01:40:40.6 + 33.4(a) OD, OH abs Hot core(4)
W28A (G5.89−0.4) 18:00:30.40 −24:04:00.0 +11.0(a) OD, OH Uncertain UCHII, hot core(3)
W31C (G10.62) 18:10:28.69 − 19:55:50.0 − 2.0(b) OD, OH abs UCHII, hot core(1)
W33A 18:14:39.52 − 17:52:00.5 + 36.7(a) OD, OH(†) UCHII, hot core(5,6)
W49N 19:10:13.20 09:06:12.0 +12.8(a) OD, OH Two comp. abs UCHII, hot core(1,3)
W51e2 19:23:43.96 14:30:34.6 + 58.2(a) OD Two comp. abs UCHII, hot core (7)
W51d 19:23:39.95 14:31:08.0 + 58.2(a) OD UCHII(1,7)
G327.29−0.6 15:53:08.55 −54:37:05.1 − 44.7(a) OD, OH abs Hot core (7)
G351.58−0.4 17:25:25.03 −36:12:45.4 − 95.9(a) OD, OH, 18OH abs UCHII, hot core(7,8)

Notes. Columns are, left to right, source designation, J2000 coordinates, LSR velocity, observed species, information on OD detection, and information on source type. (a) Based on C17O (J = 3–2) measurements with the APEX telescope from Giannetti et al. (2014) and Wyrowski et al. (2016). (b) Based on NH3 (1,1) measurements with the Effelsberg telescope from Wienen et al. (2012). (†) Only the excited OH lines have been observed.

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