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Table 1

Continuum point sources that were used for H i absorption studies.

Name RA(2000) Dec(J2000) Maj × Min T cont T cont,dif Far Scutum Spectral Location
(h:m:s) (°:′:″) (×) K K arm index

G31.3880.384 18:49:59.1 1.32.55.9 21.3 × 20.3 2055±24 20.2 yes 0.82 ext. gal
G31.411+0.307 18:47:34.1 1.12.45.5 24.0 × 23.0 914±26 19.4 no 0.63 gal.
G30.2340.138 18:47:00.4 2.27.52.9 21.7 × 20.7 853±23 42.1 no 0.00 gal.
G30.534+0.021 18:46:59.3 2.07.27.9 28.0 × 21.5a 653±21 35.9 no 0.21 gal.
G31.2420.110 18:48:44.7 1.33.13.7 25.1 × 21.2 573±22 30.1 no 0.58 gal.
G29.090+0.512 18:42:35.8 3.11.04.7 20.0 × 10.0 571±44 20.5 yes 1.03 ext. gal
G30.744+1.008 18:43:51.4 1.29.14.8 23.1 × 20.1 472±36 16.9 yes 0.90 ext. gal
G30.6990.630 18:49:36.3 2.16.27.2 22.3 × 19.6 403±18 23.4 yes 1.11 ext. gal

Notes. Continuum point sources in the observed field with brightness temperatures Tcont> 400 K. The names and spectral indexes are based on work presented in Johnston et al. (in prep.) and are preliminary results. Coordinates, major, and minor axes of the 2D fit, maximum brightness temperature Tcont of the continuum point source and the diffuse weak continuum temperature around the point source are given. The column “far Scutum arm” indicates whether absorption features at vLSR ≈ −40 km s-1 are present in the H i spectra. The spectral index and the absorption of the far Scutum arm are used to determine the location of the point sources, which is given in the last column.

(a)

This source consists of two blended sources, which explains the large eccentricity.

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