VDBH 131
(BH 131; vdBergh-Hagen 131; MWSC 2030; FSR 1615)
0.77
UTI
0.81
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
VDBH 131 is a rich, very 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, old cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~8.16 kpc) differs significantly from the median photometric distance (~5.50 kpc).
Very distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 186.545 | -63.413 | 0.123 | -6.524 | 0.288 | -30.349 |
| Hunt & Reffert | 2024 | 186.562 | -63.416 | 0.121 | -6.531 | 0.316 | -25.519 |
| Cavallo et al. | 2024 | 186.481 | -63.409 | 0.127 | â | â | â |
| He et al. | 2023 | 186.559 | -63.415 | 0.126 | -6.538 | 0.282 | -31.08 |
| Hunt & Reffert | 2023 | 186.562 | -63.416 | 0.121 | -6.531 | 0.316 | -25.519 |
| Just et al. | 2023 | 186.53 | -63.397 | â | â | â | â |
| Bica et al. | 2019 | 186.591 | -63.405 | â | â | â | â |
| Kharchenko et al. | 2016 | 186.53 | -63.397 | â | â | â | â |
| Dias et al. | 2014 | 186.558 | -63.414 | â | -5.05 | 0.06 | â |
| Kharchenko et al. | 2013 | 186.54 | -63.4 | â | -7.56 | 3.45 | â |
| Glushkova et al. | 2010 | 186.557 | -63.414 | â | â | â | â |
| Dias et al. | 2002 | 186.558 | -63.414 | â | -5.03 | 0.09 | 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 | 8912* | â | â |
| Cavallo et al. | 2024 | 5.01 | 4.10 | â | 115 | 0.010 | â | â | â |
| He et al. | 2023 | 5.50 | 4.70 | â | 158 | â | â | â | â |
| Hunt & Reffert | 2023 | 6.82 | 4.40 | 2.80 | 61 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 326 | â | â |
| Kharchenko et al. | 2016 | 4.43 | 2.58 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.43 | 2.58 | â | 1585 | â | â | â | â |
| Glushkova et al. | 2010 | 6.25 | 1.92 | â | 1259 | â | â | â | â |
| Dias et al. | 2002 | 6.25 | 1.92 | â | 1259 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Bronze sample.