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Table 1

Details of EVN observations.

Source* Pointing positions (J2000) Phase-calibrator Separation Observing Synthesized beam
Gll.ll±bb.bb RA (h m s) Dec (o′′) (.̊) run** (mas×mas,o)

G37.7600.212 19 00 55.4 04 12 12.5 J1907+0127 3.17 2 5.4×5.1;30
19 01 02.0 04 12 01.7 J1907+0127 3.15 2
G40.2800.221 19 05 41.2 06 26 12.5 J1912+0518 2.12 2 5.3×5.1;+59
G40.43+00.701 19 02 39.6 06 59 09.1 J1912+0518 3.05 1 5.6×4.7;49
G41.1200.22 19 07 14.8 07 11 00.7 J1912+0518 2.35 2 5.3×5.0;+54
G41.1600.18 19 07 11.2 07 14 04.4 J1912+0518 2.40 2 5.3×4.7;+55
G41.2300.202 19 07 21.4 07 17 08.4 J1912+0518 2.40 2 5.4×4.9;+54
G41.3500.131 19 07 21.7 07 25 17.7 J1912+0518 2.53 1 5.2×4.9;78
G43.16+00.011 19 10 11.4 09 07 06.2 J1912+0518 3.88 1
(W49N) 19 10 14.0 09 05 53.3 J1912+0518 3.86 1
19 10 14.7 09 06 16.8 J1912+0518 3.86 1 6.1×5.1;53
G45.47+00.051 19 14 25.6 11 09 27.0 J1925+1227 3.05 2 5.3×4.7;+64
G45.47+00.131 19 14 07.2 11 12 15.4 J1925+1227 3.10 2 5.3×4.7;+65
G59.78+00.071 19 43 11.1 23 44 03.0 J1931+2243 2.89 1 6.5×3.8;55

Notes. The intervals between the EVN session and the single-dish observations were (1)1–4 weeks and (2)14–15 months.

(*)

Names are the Galactic coordinates derived from the Torun survey (Szymczak et al. 2012).

(**)

2010 March 14 (run 1), 2010 March 15 (run 2).

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