VDB 1
(vdBergh 1; MWSC 934; CV Mon; OCL 527; FSR 1042)
0.85
UTI
0.62
CN
1.0
Cdens
0.62
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
74.9 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
VDB 1 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is very well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 99.278 | 3.079 | 0.552 | 0.39 | -0.702 | 9.352 |
| Almeida et al. | 2025 | 99.281 | 3.074 | β | β | β | β |
| Hunt & Reffert | 2024 | 99.273 | 3.079 | 0.554 | 0.388 | -0.711 | 9.351 |
| Cavallo et al. | 2024 | 99.282 | 3.074 | 0.555 | β | β | β |
| Hunt & Reffert | 2023 | 99.273 | 3.079 | 0.554 | 0.388 | -0.711 | 9.351 |
| Just et al. | 2023 | 99.248 | 3.071 | β | β | β | β |
| Dias et al. | 2021 | 99.281 | 3.074 | 0.521 | 0.343 | -0.786 | β |
| Cantat-Gaudin et al. | 2020 | 99.275 | 3.078 | 0.523 | 0.396 | -0.771 | β |
| SΓ‘nchez et al. | 2020 | 99.25 | 3.067 | β | 0.6 | -0.78 | β |
| Cantat-Gaudin & Anders | 2020 | 99.275 | 3.078 | 0.523 | 0.396 | -0.771 | β |
| Bica et al. | 2019 | 99.282 | 3.089 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 99.275 | 3.078 | 0.523 | 0.396 | -0.771 | β |
| Loktin & Popova | 2017 | 99.255 | 3.068 | β | -0.088 | -0.096 | 19.3 |
| Kharchenko et al. | 2016 | 99.248 | 3.071 | β | β | β | β |
| Dias et al. | 2014 | 99.25 | 3.067 | β | -0.72 | -2.76 | β |
| Kharchenko et al. | 2013 | 99.255 | 3.07 | β | -0.29 | -0.53 | 19.3 |
| Gozha et al. | 2012 | 99.25 | 3.067 | β | β | β | β |
| Kharchenko et al. | 2007 | 99.25 | 3.07 | β | 0.04 | β | β |
| van den Bergh | 2006 | 99.278 | 3.079 | β | β | β | β |
| Chen et al. | 2003 | 99.232 | 3.119 | β | -4.78 | -3.63 | 18.9 |
| Dias et al. | 2002 | 99.25 | 3.067 | β | 3.76 | -4.78 | 16.4 |
| Dambis | 1999 | 99.25 | 3.067 | β | β | β | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 1.69 | 2.26 | 2.1 | 106 | 0.444 | 188 | β | β |
| Almeida et al. | 2025 | 1.72 | 2.30 | β | 52 | β | 188 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 401(1) | β | β |
| Cavallo et al. | 2024 | 1.90 | 2.28 | β | 380 | 0.570 | β | β | β |
| Hunt & Reffert | 2023 | 1.70 | 2.37 | 2.10 | 175 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 207 | β | 166 | β | β |
| Dias et al. | 2021 | 1.72 | 2.30 | β | 52 | 0.318 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 1.95 | 1.89 | β | 41 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 1.81 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 1.81 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 1.56 | 2.12 | β | 107 | β | β | β | β |
| Kharchenko et al. | 2016 | 1.49 | 2.26 | β | 207 | β | β | β | β |
| Kharchenko et al. | 2013 | 1.49 | 2.26 | β | 207 | β | β | β | β |
| Gozha et al. | 2012 | 1.69 | β | β | 106 | β | β | β | β |
| van den Bergh | 2006 | 1.69 | 2.20 | β | 105 | β | β | β | β |
| Chen et al. | 2003 | 1.69 | β | β | 100 | β | β | β | β |
| Dias et al. | 2002 | 1.69 | 2.20 | β | 106 | β | β | β | β |
| Dambis | 1999 | 1.45 | 2.12 | β | 79 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.