Berkeley 90
(MWSC 3377)
0.81
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
4.3 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Berkeley 90 is a rich, 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, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 308.818 | 46.843 | 0.333 | -2.869 | -4.364 | -45.116 |
| Hunt & Reffert | 2024 | 308.812 | 46.844 | 0.343 | -2.875 | -4.367 | -19.413 |
| Celli et al. | 2024 | 308.819 | 46.843 | â | â | â | â |
| Cavallo et al. | 2024 | 308.823 | 46.841 | 0.342 | â | â | â |
| Hunt & Reffert | 2023 | 308.812 | 46.844 | 0.343 | -2.875 | -4.367 | -19.413 |
| Just et al. | 2023 | 308.807 | 46.838 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 308.819 | 46.843 | 0.302 | -2.829 | -4.369 | â |
| Cantat-Gaudin & Anders | 2020 | 308.819 | 46.843 | 0.302 | -2.829 | -4.369 | â |
| Cantat-Gaudin et al. | 2018 | 308.819 | 46.843 | 0.302 | -2.829 | -4.369 | â |
| Loktin & Popova | 2017 | 308.805 | 46.841 | â | -0.267 | -0.155 | â |
| Kharchenko et al. | 2016 | 308.807 | 46.838 | â | â | â | â |
| Dias et al. | 2014 | 308.825 | 46.833 | â | -2.13 | -0.52 | â |
| Kharchenko et al. | 2013 | 308.812 | 46.841 | â | -2.09 | -0.63 | â |
| Dias et al. | 2002 | 308.825 | 46.833 | â | -2.13 | -0.52 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1923* | â | â |
| Celli et al. | 2024 | â | â | â | 5 | â | 817 | â | â |
| Cavallo et al. | 2024 | 2.50 | 3.85 | â | 45 | 0.420 | â | â | â |
| Hunt & Reffert | 2023 | 2.76 | 3.90 | 2.82 | 8 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 200 | â | 385 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.02 | 3.60 | â | 5 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.02 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.02 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 1.63 | 2.03 | â | 1047 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.65 | 3.68 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.65 | 3.68 | â | 200 | â | â | â | â |
| Dias et al. | 2002 | 2.07 | 3.69 | â | 112 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.