ESO 211 09
(MWSC 1646)
0.68
UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
0.9 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
ESO 211 09 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Very distant
High extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 139.188 | -50.289 | 0.132 | -3.455 | 3.08 | 70.483 |
| Just et al. | 2023 | 139.179 | -50.279 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 139.186 | -50.285 | 0.093 | -3.53 | 3.12 | â |
| Cantat-Gaudin & Anders | 2020 | 139.186 | -50.285 | 0.093 | -3.53 | 3.12 | â |
| Soubiran et al. | 2018 | 139.186 | -50.285 | â | â | â | 52.08 |
| Cantat-Gaudin et al. | 2018 | 139.186 | -50.285 | 0.093 | -3.53 | 3.12 | â |
| Kharchenko et al. | 2016 | 139.179 | -50.279 | â | â | â | â |
| Dias et al. | 2014 | 139.183 | -50.285 | â | -3.91 | 8.45 | â |
| Kharchenko et al. | 2013 | 139.183 | -50.283 | â | -3.71 | 9.04 | â |
| Dias et al. | 2002 | 139.183 | -50.285 | â | -3.71 | 9.04 | â |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 501 | â | 14 | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.18 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 8.18 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.18 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.15 | 3.23 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.15 | 3.23 | â | 501 | â | â | â | â |
| Dias et al. | 2002 | 5.82 | 3.47 | â | 1122 | â | â | â | â |

