Kronberger 54
(MWSC 3237; DSH J2003.1+3158)
0.77
UTI
0.62
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
50.9 [N/pc2]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
Kronberger 54 is a moderately populated, very 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 and mass parameters (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 | 99999â | 300.779 | 31.966 | 0.217 | -2.638 | -5.219 | -8.8 |
| Hunt & Reffert | 2024 | 300.781 | 31.964 | 0.231 | -2.652 | -5.189 | -8.829 |
| Cavallo et al. | 2024 | 300.781 | 31.958 | 0.228 | â | â | â |
| Hunt & Reffert | 2023 | 300.781 | 31.964 | 0.231 | -2.652 | -5.189 | -8.829 |
| Just et al. | 2023 | 300.778 | 31.965 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 300.778 | 31.968 | 0.195 | -2.596 | -5.209 | â |
| Cantat-Gaudin & Anders | 2020 | 300.778 | 31.968 | 0.195 | -2.596 | -5.209 | â |
| Bica et al. | 2019 | 300.784 | 31.97 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 300.778 | 31.968 | 0.195 | -2.596 | -5.209 | â |
| Kharchenko et al. | 2016 | 300.778 | 31.965 | â | â | â | â |
| Kharchenko et al. | 2013 | 300.783 | 31.967 | â | -4.2 | -3.35 | â |
| Bukowiecki et al. | 2011 | 300.783 | 31.969 | â | â | â | â |
| Kronberger et al. | 2006 | 300.783 | 31.967 | â | â | â | â |
| Dias et al. | 2002 | 300.783 | 31.967 | â | -4.2 | -3.35 | 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 | 4.055 | 2.84 | 2.76 | 447 | 0.180 | 90 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1399(1) | â | â |
| Cavallo et al. | 2024 | 3.77 | 3.58 | â | 11 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 4.34 | 3.96 | 2.76 | 11 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 676 | â | 71 | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.46 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.46 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.90 | 2.77 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.90 | 2.77 | â | 676 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 90 | â | â |
| Bukowiecki et al. | 2011 | 6.05(1) | 2.45 | â | 447 | â | â | â | â |
| Dias et al. | 2002 | 1.72 | 2.91 | â | 251 | 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)
Silver sample.