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Table 2

Results of EVN observations.

Sourcea Position of the brightest spot (J2000) Vp ΔV Sp Dnear/Dfar Dadopted Classb
Gll.lll ± bb.bbb RA (h m s) Dec (°′′) (km s-1) (km s-1) (Jy beam-1) (kpc) (kpc)

G20.237+00.065 18 27 44.56429 11 14 54.0938 71.8 9.4 22.98 4.4/11.2 4.4d C
G20.239+00.065 18 27 44.95441 11 14 47.8165 61.0 11.0 2.41 3.9/11.7 L
G22.43500.169 18 32 43.81865 09 24 32.7838 29.3 16.6 2.44 2.2/13.1 R
G23.01000.411 18 34 40.28623 09 00 38.1037 74.7 11.6 72.6 4.3/11.0 4.59e C
G24.33+00.14c1 18 35 08.119 07 35 04.13 110.3 5.6 1.62 5.7/9.5 9.5d C
G24.49400.038 18 36 05.72977 07 31 19.2012 115.1 8.3 2.85 5.8/9.3 C
G24.790+00.083 18 36 12.56216 07 12 10.8211 113.4 10.5 55.83 5.8/9.4 7.7f (P)R, R
G24.850+00.087 18 36 18.38754 07 08 50.8051 110.2 7.9 5.9 5.7/9.5 8.0g C
G28.01100.426 18 43 57.96865 04 34 24.0938 16.1 12.7 1.26 1.1/13.4 C
G29.97800.048 18 46 12.96122 02 39 01.3798 103.5 8.9 31.2 5.6/8.8 8.8d C
G30.19800.169 18 47 03.07004 02 30 36.2597 108.2 10.4 14.7 5.9/8.5 C
G30.22400.180 18 47 08.29781 02 29 29.3199 113.4 3.0 2.58 6.6/7.9 C
G32.74400.076c2 18 51 21.8671 00 12 05.3 33.4 11.1 10.5 2.3/11.8 11.8d (P)A, L
G34.245+00.134 18 53 21.45175 +01 13 46.0317 55.0 8.2 1.4 3.3/10.4 3.3h C
G34.258+00.153 18 53 18.64476 +01 15 00.4115 57.6 1.8 5.9 3.4/10.3 3.4h C
G34.396+00.222 18 53 19.09345 +01 24 13.862 55.6 7.8 5.2 3.3/10.4 3.6i C
G35.025+00.350 18 54 00.65696 +02 01 19.3260 43.9 5.5 5.3 2.7/10.9 2.32j L

Notes. Coordinates with less accuracy (see Sect. 2.3): and Distances derived from trigonometric parallaxes by Kinematic distance ambiguity resolved from: In the remaining targets the near kinematic distances were assumed.

(a)

Names are the Galactic coordinates derived from the EVN results.

(b)

Class of morphology as described in Bartkiewicz et al. (2009): L – linear, R – ring, C – complex, A – arched, P – pair.

(c1)

from the BeSSeL survey (EVLA) by Hu et al., (in prep.)

(c2)

estimated from uncleaned EVN images with uncertainties of ΔRA = 00005 and ΔDec = 1.̋7.

(e)

Brunthaler et al. (2009),

(j)

Wu et al. (2014).

(d)

Green & McClure-Griffiths (2011),

(f)

Moscadelli et al. (2007),

(g)

Hill et al. (2005),

(h)

Kuchar & Bania (1994),

(i)

He et al. (2012).

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