Summary table of the four velocity ranges in which is divided the dust emission of the G332 Galactic plane sector. The mean N(H2) is traced from the fractional dust emission as described in the Section 10.1. The distance is computed from the VLSR value of the centroid velocity of each interval.
| Interval . | Distance . | Mass . | Mean N(HI) . | Mean N(H2) . |
|---|---|---|---|---|
| . | kpc . | M⊙ . | 1020 cm−2 . | 1020 cm−2 . |
| R1 | 8.8 | 12.2 × 105 | 13.0 | 100 |
| R2 | 10.5 | 6.6 × 105 | 6.9 | 54 |
| R3 | 3.7 | 2.00 × 105 | 6.1 | 95 |
| R4 | 2.9 | 0.5 × 105 | 4.6 | 56 |
| Interval . | Distance . | Mass . | Mean N(HI) . | Mean N(H2) . |
|---|---|---|---|---|
| . | kpc . | M⊙ . | 1020 cm−2 . | 1020 cm−2 . |
| R1 | 8.8 | 12.2 × 105 | 13.0 | 100 |
| R2 | 10.5 | 6.6 × 105 | 6.9 | 54 |
| R3 | 3.7 | 2.00 × 105 | 6.1 | 95 |
| R4 | 2.9 | 0.5 × 105 | 4.6 | 56 |
Summary table of the four velocity ranges in which is divided the dust emission of the G332 Galactic plane sector. The mean N(H2) is traced from the fractional dust emission as described in the Section 10.1. The distance is computed from the VLSR value of the centroid velocity of each interval.
| Interval . | Distance . | Mass . | Mean N(HI) . | Mean N(H2) . |
|---|---|---|---|---|
| . | kpc . | M⊙ . | 1020 cm−2 . | 1020 cm−2 . |
| R1 | 8.8 | 12.2 × 105 | 13.0 | 100 |
| R2 | 10.5 | 6.6 × 105 | 6.9 | 54 |
| R3 | 3.7 | 2.00 × 105 | 6.1 | 95 |
| R4 | 2.9 | 0.5 × 105 | 4.6 | 56 |
| Interval . | Distance . | Mass . | Mean N(HI) . | Mean N(H2) . |
|---|---|---|---|---|
| . | kpc . | M⊙ . | 1020 cm−2 . | 1020 cm−2 . |
| R1 | 8.8 | 12.2 × 105 | 13.0 | 100 |
| R2 | 10.5 | 6.6 × 105 | 6.9 | 54 |
| R3 | 3.7 | 2.00 × 105 | 6.1 | 95 |
| R4 | 2.9 | 0.5 × 105 | 4.6 | 56 |
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