Kronberger 57
(MWSC 3330; DSH J2023.9+3636; FSR 0206)
0.78
UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
1.3 [arcmin]
- CN 0.58 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
Kronberger 57 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~3.54 kpc) differs significantly from the median photometric distance (~2.43 kpc).
Relatively close
High extinction
Metal-rich
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 305.989 | 36.602 | 0.282 | -3.55 | -4.417 | -35.082 |
| Hunt & Reffert | 2024 | 305.988 | 36.603 | 0.283 | -3.564 | -4.438 | â |
| Cavallo et al. | 2024 | 305.992 | 36.604 | 0.277 | â | â | â |
| Hunt & Reffert | 2023 | 305.988 | 36.603 | 0.283 | -3.564 | -4.438 | â |
| Just et al. | 2023 | 305.983 | 36.598 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 305.986 | 36.602 | 0.275 | -3.54 | -4.406 | â |
| Cantat-Gaudin & Anders | 2020 | 305.986 | 36.602 | 0.275 | -3.54 | -4.406 | â |
| Bica et al. | 2019 | 305.989 | 36.607 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 305.986 | 36.602 | 0.275 | -3.54 | -4.406 | â |
| Loktin & Popova | 2017 | 305.985 | 36.6 | â | -0.379 | -0.973 | â |
| Kharchenko et al. | 2016 | 305.983 | 36.598 | â | â | â | â |
| Dias et al. | 2014 | 305.987 | 36.605 | â | -3.3 | -10.03 | â |
| Kharchenko et al. | 2013 | 305.988 | 36.6 | â | -2.35 | -2.01 | â |
| Kronberger et al. | 2006 | 305.99 | 36.605 | â | â | â | â |
| Dias et al. | 2002 | 305.988 | 36.605 | â | -2.35 | -2.01 | 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 | 1068* | â | â |
| Cavallo et al. | 2024 | 2.78 | 5.38 | â | 9 | 0.610 | â | â | â |
| Hunt & Reffert | 2023 | 3.01 | 5.49 | 2.66 | 99 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 891 | â | 4 | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.29 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.29 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.09 | 3.57 | â | 170 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.76 | 4.58 | â | 891 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.76 | 4.58 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 1.29 | 3.29 | â | 158 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.