VDBH 222
(vdBergh-Hagen 222; MWSC 2564; BH 222; ESO 333 04)
0.82
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.6 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 222 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as an extremely massive, near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
Very distant
Very high extinction
Extremely massive
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 259.695 | -38.287 | 0.139 | -1.919 | -3.167 | -113.0 |
| Hunt & Reffert | 2024 | 259.645 | -38.425 | 0.426 | -0.223 | -1.059 | -42.259 |
| Cavallo et al. | 2024 | 259.657 | -38.433 | 0.428 | â | â | â |
| Hunt & Reffert | 2023 | 259.645 | -38.425 | 0.426 | -0.223 | -1.059 | -42.259 |
| Just et al. | 2023 | 259.678 | -38.295 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 259.694 | -38.289 | 0.114 | -2.091 | -3.192 | â |
| Cantat-Gaudin & Anders | 2020 | 259.694 | -38.289 | 0.114 | -2.091 | -3.192 | â |
| Soubiran et al. | 2018 | 259.694 | -38.289 | â | â | â | -119.29 |
| Bica et al. | 2019 | 259.689 | -38.288 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 259.694 | -38.289 | 0.114 | -2.091 | -3.192 | â |
| Kharchenko et al. | 2016 | 259.678 | -38.295 | â | â | â | â |
| Dias et al. | 2014 | 259.696 | -38.283 | â | -1.44 | -3.27 | â |
| Kharchenko et al. | 2013 | 259.687 | -38.295 | â | -1.31 | -2.92 | â |
| van den Bergh | 2006 | 259.7 | -38.283 | â | â | â | â |
| Dias et al. | 2002 | 259.696 | -38.283 | â | -2.59 | -4.05 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 762* | â | â |
| Cavallo et al. | 2024 | 1.57 | 3.96 | â | 10 | -0.480 | â | â | â |
| Hunt & Reffert | 2023 | 2.17 | 3.85 | 2.31 | 14 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 79 | â | 717794 | â | â |
| Cantat-Gaudin & Anders | 2020 | 6.98 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 6.98 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 6.98 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 7.81 | 5.16 | â | 79 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.81 | 5.16 | â | 79 | â | â | â | â |
| van den Bergh | 2006 | 6.00 | 5.74 | â | 60 | â | â | â | â |
| Dias et al. | 2002 | 6.00 | 5.74 | â | 60 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.