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Table 1

Summary of sources.

Source name RA α (J2000) Dec δ (J2000) υsys (kms−1) SiO (1−0) H2O maser CH3OH maser Selected category ATLASGAL name Classification
IRAS18032−2032 18:06:14 −20:31:47 5.0 Y(b) Y Y UCHII 009.621+00.194 MSF (radio-HII)w
G8.67−0.36 18:06:19 −21:37:32 38.0 Y(b) Y Y UCHII 008.671−00.356 MSF (radio-HII)w
G10.47+0.03 18:08:38 −19:51:52 66.2 Y(b) Y Y UCHII 010.472+00.027 MSF (radio-HII)w
G10.30−0.15 18:08:56 −20:05:54 11.0 Y(b) Y Y UCHII 010.299−00.147 MSF (radio-HII)w
G10.15−0.34 18:09:25 −20:19:15 5.0 N N N UCHII MSF (radio-HII)w
IRAS18073−2046 18:10:17 −20:45:43 28.0 N Y Y UCHII 009.879−00.751 MSF (radio-HII)w
G10.62−0.38 18:10:24 −19:56:15 −3.0 N Y Y UCHII MSF (radio-HII)w
IRAS18085−1931 18:11:33 −19:30:39 −1.1 Y(e) N N UCHII 011.109−00.397 MSF (radio-HII)w
HM18089−1732 18:11:51 −17:31:28 33.0 Y(c) Y Y HMPO 012.888+00.489 MSF (radio-HII)
HM18090−1832 18:12:02 −18:31:56 110.0 N N N HMPO 012.024−00.031 YSO
G12.21−0.10 18:12:40 −18:24:21 20.0 Y(b,c) Y Y UCHII 012.208−00.102 MSF (radio-HII)w
G12.43−0.05 18:12:55 −18:11:08 40.0 N N N UCHII 012.431−00.049 MSF (radio-HII)w
HM18102−1800 18:13:12 −17:59:35 21.0 Y(b) N Y HMPO unclassified
G11.94−0.62 18:14:01 −18:53:24 38.9 Y(b,c) Y Y UCHII 011.936−00.616 MSF (radio-HII)w
HM18144−1723 18:17:24 −17:22:13 47.0 Y(a,c) Y Y HMPO 013.658−00.599 YSO
G015.05+00.07 MM2 18:17:40 −15:48:55 24.7 N N N IRDC 015.053+00.089 YSO
G015.05+00.07 MM1 18:17:50 −15:53:38 24.7 Y(d) N N IRDC 015.006+00.009 Quiescent
HM18151−1208 18:17:57 −12:07:22 33.0 Y(e) Y Y HMPO unclassified
HM18159−1550 18:18:48 −15:48:54 60.0 N N N HMPO 015.184−00.159 MSF (HII)
G015.31−00.16MM2 18:18:50 −15:43:19 31.1 N N N IRDC 015.271−00.122 Protostellar
G015.31−00.16MM1 18:18:56 −15:45:00 31.1 N N N IRDC unclassified

Notes. This table only shows a fraction of the whole table; the full table is available at the CDS. υsys is systemic velocity, and the velocity information is obtained from several molecular line observations (NH3; Churchwell et al. 1990; Molinari et al. 1996; Beuther et al. 2002; Chira et al. 2013; CS; Bronfman et al. 1996). (*)UCHII sources without ATLASGAL classification. The presence of SiO wings in rotational transitions, 1–0 from this survey and 2–1 from the survey presented in Csengeri et al. (2016a) are indicated with four different classifications:(a) indicates wing features in SiO 1–0 emission, and (b) means SiO wing candidates for cases with a SiO FWHM ≥8 kms,(c) indicates SiO wings in the 2–1 transition, and (d) is for the cases that there are no wings in 2–1 transition but a broad Gaussian component has a FWHM line width ≥ 8 kms, (e) marks for sources without any sign of wing features in either 1–0 or 2–1 transitions.

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