VDBH 67
(vdBergh-Hagen 67; MWSC 1669; BH 67; ESO 212 07; FSR 1486)
0.80
UTI
0.86
CN
1.0
Cdens
0.62
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
1.8 [arcmin]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
VDBH 67 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Very distant
High extinction
Massive
Metal-rich
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 141.682 | -51.275 | 0.132 | -3.676 | 2.901 | 49.601 |
| Hunt & Reffert | 2024 | 141.684 | -51.273 | 0.109 | -3.683 | 2.871 | 56.588 |
| Cavallo et al. | 2024 | 141.691 | -51.268 | 0.118 | β | β | β |
| Hunt & Reffert | 2023 | 141.684 | -51.273 | 0.109 | -3.683 | 2.871 | 56.588 |
| Just et al. | 2023 | 141.677 | -51.269 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 141.687 | -51.273 | 0.098 | -3.64 | 2.811 | β |
| SΓ‘nchez et al. | 2020 | 141.688 | -51.267 | β | -3.486 | 2.792 | β |
| Cantat-Gaudin & Anders | 2020 | 141.687 | -51.273 | 0.098 | -3.64 | 2.811 | β |
| Bica et al. | 2019 | 141.695 | -51.263 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 141.687 | -51.273 | 0.098 | -3.64 | 2.811 | β |
| Kharchenko et al. | 2016 | 141.677 | -51.269 | β | β | β | β |
| Dias et al. | 2014 | 141.688 | -51.267 | β | -6.38 | 3.86 | β |
| Kharchenko et al. | 2013 | 141.682 | -51.273 | β | -7.31 | 5.72 | β |
| Dias et al. | 2002 | 141.688 | -51.267 | β | -6.38 | 3.86 | β |
π‘ 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 | β | β | β | β | β | 754* | β | β |
| Cavallo et al. | 2024 | 8.83 | 3.37 | β | 692 | 0.700 | β | β | β |
| Hunt & Reffert | 2023 | 6.95 | 3.50 | 1.43 | 71 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 684 | β | 2234 | β | β |
| Cantat-Gaudin et al. | 2020 | 8.17 | 3.00 | β | 617 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 7.89 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 7.89 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 6.50 | 3.23 | β | 684 | β | β | β | β |
| Kharchenko et al. | 2013 | 6.50 | 3.23 | β | 684 | β | β | β | β |
| Dias et al. | 2002 | 7.50 | 2.94 | β | 1288 | β | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.