Berkeley 84
(MWSC 3241)
0.61
UTI
0.58
CN
0.74
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Stellar density (N50/rad)
3.7 [N/pc2]
- CN 0.58 Moderately populated
- Cdens 0.74 Moderately dense
- CC3 0.75 High quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
Berkeley 84 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate* distance, above 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 moderately studied in the literature.
(*): The parallax distance estimate (~2.79 kpc) differs significantly from the median photometric distance (~2.10 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 301.196 | 33.949 | 0.358 | -2.008 | -5.551 | 11.22 |
| Hunt & Reffert | 2024 | 301.2 | 33.986 | 0.352 | -2.012 | -5.555 | 54.163 |
| Cavallo et al. | 2024 | 301.193 | 33.983 | 0.357 | â | â | â |
| Hunt & Reffert | 2023 | 301.2 | 33.986 | 0.352 | -2.012 | -5.555 | 54.163 |
| Just et al. | 2023 | 301.165 | 33.903 | â | â | â | â |
| Loktin & Popova | 2017 | 301.185 | 33.907 | â | -3.329 | -0.703 | â |
| Kharchenko et al. | 2016 | 301.165 | 33.903 | â | â | â | â |
| Dias et al. | 2014 | 301.179 | 33.907 | â | -0.24 | -4.5 | â |
| Kharchenko et al. | 2013 | 301.17 | 33.906 | â | -2.09 | -0.41 | â |
| Dias et al. | 2002 | 301.179 | 33.907 | â | -2.09 | -0.41 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.095 | 2.16 | 2.86 | 120 | 0.350 | 345 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 568(1) | â | â |
| Cavallo et al. | 2024 | 2.14 | 2.06 | â | 269 | 0.350 | â | â | â |
| Hunt & Reffert | 2023 | 2.49 | 1.98 | 2.86 | 47 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 120 | â | 122 | â | â |
| Loktin & Popova | 2017 | 1.97 | 0.99 | â | 1148 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.05 | 2.36 | â | 120 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.05 | 2.36 | â | 120 | â | â | â | â |
| Dias et al. | 2002 | 2.75 | 2.26 | â | 447 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.