VDBH 151
(BH 151)
0.74
UTI
0.64
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
1.2 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
VDBH 151 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Distant
High extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 205.051 | -61.733 | 0.226 | -5.874 | -1.851 | 37.294 |
| Almeida et al. | 2025 | 205.05 | -61.732 | â | â | â | â |
| Hunt & Reffert | 2024 | 205.044 | -61.728 | 0.254 | -5.889 | -1.782 | 105.015 |
| Celli et al. | 2024 | 205.051 | -61.731 | â | â | â | â |
| Cavallo et al. | 2024 | 205.039 | -61.733 | 0.25 | â | â | â |
| Hunt & Reffert | 2023 | 205.044 | -61.728 | 0.254 | -5.889 | -1.782 | 105.015 |
| Dias et al. | 2021 | 205.05 | -61.732 | 0.159 | -5.867 | -1.87 | â |
| Cantat-Gaudin et al. | 2020 | 205.051 | -61.731 | 0.176 | -5.853 | -1.878 | â |
| Cantat-Gaudin & Anders | 2020 | 205.051 | -61.731 | 0.176 | -5.853 | -1.878 | â |
| Monteiro & Dias | 2019 | 205.051 | -61.731 | â | -5.858 | -1.874 | 2.787 |
| Cantat-Gaudin et al. | 2018 | 205.051 | -61.731 | 0.176 | -5.853 | -1.878 | â |
| Dias et al. | 2002 | 205.046 | -61.731 | â | 0.05 | -6.2 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.87 | 4.10 | â | 6 | â | 489 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1017* | â | â |
| Celli et al. | 2024 | â | â | â | 16 | â | 418 | â | â |
| Cavallo et al. | 2024 | 2.67 | 4.49 | â | 16 | 0.820 | â | â | â |
| Hunt & Reffert | 2023 | 3.95 | 4.82 | 2.86 | 13 | â | â | â | â |
| Dias et al. | 2021 | 3.87 | 4.10 | â | 6 | 0.341 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.99 | 4.06 | â | 16 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.88 | â | â | â | â | â | â | â |
| Monteiro & Dias | 2019 | 4.42 | 3.81 | â | 7 | 0.030 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.88 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 3.80 | â | â | â | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Bronze sample.