Table 3
Properties of the five largest 13CO velocity-coherent structures identified in G202.3+2.5.
Id | RA | Dec | ⟨vlsr ⟩ | Area | Δθmin | Δθmax | e | Δvlsr | ⟨Tmb⟩ | σ(Tmb) | ⟨N(H2)⟩ | M |
---|---|---|---|---|---|---|---|---|---|---|---|---|
(h m s) | (d m s) | (km s−1) | (arcmin2) | (′) | (′) | (km s−1) | (K) | (K) | (cm−2) | (M⊙) | ||
1 | 06 40 59.7 | 10 32 36.5 | 7.77 | 25.72 | 3.54 | 8.75 | 2.47 | 1.92 | 7.76 | 1.84 | 10.5(21) | 292 |
2 | 06 41 05.9 | 10 40 03.6 | 6.27 | 23.58 | 3.13 | 9.75 | 3.12 | 1.68 | 5.52 | 1.19 | 7.9(21) | 203 |
3 | 06 41 01.0 | 10 40 02.4 | 8.63 | 10.26 | 1.96 | 6.96 | 3.55 | 1.80 | 6.74 | 1.29 | 7.5(21) | 84 |
4 | 06 40 54.6 | 10 48 11.3 | 8.55 | 7.14 | 1.21 | 6.54 | 5.41 | 1.62 | 6.30 | 1.33 | 5.5(21) | 43 |
5 | 06 40 53.1 | 10 53 25.4 | 5.51 | 17.95 | 3.21 | 8.83 | 2.75 | 1.20 | 4.77 | 0.81 | 5.2(21) | 103 |
Notes. The columns are, for each component: (1) the identity index; (2–3) the central coordinates; (4) the average radial velocity; (5) the total area inthe plane of the sky; (6–7) the minimum and maximum extent; (8) the elongation, computed as the ratio of the two previous columns; (9) the velocity extent, computed as the difference between the minimum and maximum vlsr of the component; (10) the mean 13CO main-beam temperature; (11) the standard deviation of 13CO brightness temperature; (12) the mean column density from 13CO emission, where (21) means 1021 ; (13) the mass from 13CO emission.
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