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Table 1

Source coordinates and basic physical parameters.

Source RAa (h : m : s) Deca (◦ : ′ : ″) VLSRb (km s−1) db (kpc) Lb (L) N(H2)c (cm−2)
HMSC
G034G2(MM2) [G034] 18:56:50.0 01:23:08 +43.6 2.9 101.6 4.1×1022
HMPO
AFGL5142–MM [AFGL] 05:30:48.0 33:47:54 −3.9 1.8 103.6 1.0×1023
UCHII
G5.89–0.39 [G589] 18:00:30.5 −24:04:01 +9.0 1.3 105.1 5.5 × 1023

Notes. (a) J2000. (b) Derived from either observations of 13CO (G034) or NH3 inversion transitions (AFGL, G589). Reference works in Fontani et al. (2011). (c) From Fontani et al. (2018), computed from the dust thermal continuum emission images at 850 μm obtained with the Submillimeter Common-User Bolometer Array (SCUBA) at the James Clerk Maxwell Telescope (JCMT) by Di Francesco et al. (2008).

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