Open Access
Table A.11.
Vela molecular ridge extra candidate member properties.
1 | 2 | 3 | 4 | 5 | 6 | 7 | 8 | 9 | 10 | 11 | 12 | 13 |
---|---|---|---|---|---|---|---|---|---|---|---|---|
OSC | OC | l | b | plx | d | ![]() |
μδ | R | N | Age | RV | Ref |
Acronym | Name | degree | degree | mas | kpc | mas/yr | mas/yr | arcmin | stars | Myr | km/s | |
Vela | Pismis 5 | 259.36 | 0.91 | 1.03 | 0.94 | -5.5 | 4.3 | 7.4a | 80 | 10 | CG20 | |
molecular | ||||||||||||
ridge | ||||||||||||
Casado-Hendy 3 | 266.97 | 1.64 | 1.01 | 0.95 | -5.7 | 4.9 | 43b | 30 | 20 | 20 | TW | |
±0.09 | ±0.04 | ±0.2 | ±0.3 | ±2 | ±6 |
Notes. Column headings are as in Table A.2. References (CG20 (Cantat-Gaudin et al. 2020); TW (This Work)). Abbreviations: a radius containing 50% of members; b maximum cluster member distance to the average position.
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