Table 1
Properties of studied filament regions.
| (1) | (2) | (3) | (4) | (5) | (6) |
|---|---|---|---|---|---|
| Source name (a) | Glon(º.º) | Glat (º.º) | υLSR (km s−1) | dnear (b) (kpc) | DGC (b) (kpc) |
| GMF20.0-17.9 | 17.80–20.60 | −1.00–+0.30 | 37–50 | 3.2 | 5.2 |
| GMF26.7-25.4 | 25.10–26.90 | +0.40–+1.20 | 41–51 | 2.9 | 5.7 |
| GMF38.1-32.4a | 33.30–37.30 | −1.00–+0.60 | 50–60 | 3.2 | 5.9 |
| GMF38.1-32.4b | 33.30–37.30 | −1.00–+0.60 | 43–46 | 2.6 | 6.2 |
| GMF41.0-41.3 | 40.80–41.50 | −0.70–+0.50 | 34–42 | 2.2 | 6.7 |
| GMF54.0-52.0 | 52.30–54.20 | −0.50–+0.40 | 20–26 | 1.4 | 7.4 |
Notes. Columns (2) and (3) give the Galactic longitude range and latitude range of the filament regions, respectively. Column (4) gives the line-of-sight velocity range of each GMF as defined in Ragan et al. (2014). Columns (5) and (6) give the kinematic near distance from us and the Galactocentric distance, respectively.(a) As in Ragan et al. (2014). (b)The distances are not taken from Ragan et al. (2014) but have been recalculated using the more recent spiral arm model by Reid et al. (2019).
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