Table 3
Sources coordinates, heliocentric distances, line-of-sight velocities, and evolutionary phases (e.p.).
Source | α(J2000) | δ(J2000) | l | b | d | vLSR | e.p. | |
---|---|---|---|---|---|---|---|---|
[h m s] | [° ′ ′′] | [°] | [°] | [kpc] | [km s−1] | |||
1 | I00117–MM1 | 00 14 26.1 | +64 28 44.0 | 118.96 | +1.89 | 1.8(a) | −36.3 | HMPO |
2 | I00117–MM2 | 00 14 26.3 | +64 28 28.0 | 118.96 | +1.89 | 1.8(a) | −36.3 | HMSC |
3 | AFGL5142–MM | 05 30 48.0 | +33 47 54.0 | 174.20 | −0.07 | 1.8(b) | −3.9 | HMPO |
4 | AFGL5142–EC | 05 30 48.7 | +33 47 53.0 | 174.20 | −0.07 | 1.8(b) | −3.9 | HMSC(w) |
5 | 05358–mm3 | 05 39 12.5 | +35 45 55.0 | 173.48 | +2.45 | 1.8(b) | −17.6 | HMSC(w) |
6 | 05358–mm1 | 05 39 13.1 | +35 45 51.0 | 173.48 | +2.45 | 1.8(b) | −17.6 | HMPO |
7 | G5.89–0.39 | 18 00 30.5 | −24 04 01.0 | 5.89 | −0.39 | 1.3(b) | +9.0 | UC HII |
8 | G008.14+0.22 | 18 03 01.3 | −21 48 05.0 | 8.14 | +0.22 | 3.4(c) | +20.1 | |
9 | 18089−1732M1 | 18 11 51.4 | −17 31 28.0 | 12.89 | +0.49 | 3.6(b),(*) | +32.7 | HMPO |
10 | 18089−1732 M4 | 18 11 54.0 | −17 29 59.0 | 12.92 | +0.49 | 3.6(d),(*) | +33.8 |
Notes. For the sources present in the Hi-GAL catalog the distance values were taken from Elia et al. (2017) (distance match < 10′′). The sources of Subsample I present an evolutionary classification in Col. 9, while for sources of Subsample II column 9 is empty. For the other sources: (a) Molinari et al. (1996); (b) Fontani et al. (2011); (c) Faúndez et al. (2004); (d) Sridharan et al. (2002). (*) Ambiguity in the distance estimate not resolved, theadopted distance is the dnear; (**) during observations vLSR differed from the correct value reported in this table. (w)HMSC defined as warm (Fontani et al. 2011). The full table is available at the CDS.
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