VDBH 110
(BH 110; vdBergh-Hagen 110; MWSC 1894)
0.57
UTI
0.45
CN
0.89
Cdens
0.75
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
1.1 [arcmin]
- CN 0.45 Poorly populated
- Cdens 0.89 Dense
- CC3 0.75 High quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
VDBH 110 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a large* distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~9.95 kpc) differs significantly from the median photometric distance (~5.59 kpc).
Very distant
Moderate extinction
Massive
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 166.763 | -61.509 | 0.101 | -5.913 | 2.207 | 41.859 |
| Hunt & Reffert | 2024 | 166.771 | -61.51 | 0.107 | -5.918 | 2.207 | 30.086 |
| Cavallo et al. | 2024 | 166.755 | -61.496 | 0.106 | â | â | â |
| Hunt & Reffert | 2023 | 166.771 | -61.51 | 0.107 | -5.918 | 2.207 | 30.086 |
| Bica et al. | 2019 | 166.767 | -61.513 | â | â | â | â |
| Dias et al. | 2014 | 166.825 | -61.45 | â | -0.94 | -3.4 | â |
| Dias et al. | 2002 | 166.825 | -61.45 | â | -9.28 | 2.1 | 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 | 1604* | â | â |
| Cavallo et al. | 2024 | 5.40 | 2.55 | â | 155 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 8.30 | 3.07 | 2.47 | 28 | â | â | â | â |
| Dias et al. | 2002 | 5.59 | 1.30 | â | 1000 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.