Berkeley 83
(MWSC 3223; OCL 135; FSR 0171)
0.79
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
1.4 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Berkeley 83 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Very distant
High 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 | 300.361 | 28.643 | 0.123 | -2.643 | -4.726 | 0.291 |
| Hunt & Reffert | 2024 | 300.356 | 28.643 | 0.153 | -2.677 | -4.804 | â |
| Cavallo et al. | 2024 | 300.372 | 28.658 | 0.158 | â | â | â |
| Hunt & Reffert | 2023 | 300.356 | 28.643 | 0.153 | -2.677 | -4.804 | â |
| Just et al. | 2023 | 300.354 | 28.628 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 300.356 | 28.645 | 0.092 | -2.604 | -4.692 | â |
| Cantat-Gaudin & Anders | 2020 | 300.356 | 28.645 | 0.092 | -2.604 | -4.692 | â |
| Bica et al. | 2019 | 300.353 | 28.641 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 300.356 | 28.645 | 0.092 | -2.604 | -4.692 | â |
| Kharchenko et al. | 2016 | 300.354 | 28.628 | â | â | â | â |
| Dias et al. | 2014 | 300.325 | 28.617 | â | -3.01 | 0.44 | â |
| Kharchenko et al. | 2013 | 300.36 | 28.63 | â | -3.03 | -6.91 | â |
| Dias et al. | 2002 | 300.325 | 28.617 | â | -3.03 | -6.91 | 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 | 1849* | â | â |
| Cavallo et al. | 2024 | 5.94 | 4.88 | â | 240 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 4.95 | 5.49 | 2.21 | 299 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 484 | â | 4325 | â | â |
| Cantat-Gaudin et al. | 2020 | 6.67 | 4.59 | â | 240 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.26 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.26 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 7.84 | 5.10 | â | 484 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.84 | 5.10 | â | 484 | 0.000 | â | â | â |
| Dias et al. | 2002 | 5.73 | 4.03 | â | 891 | 0.000 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.