Kronberger 52
(MWSC 3211; DSH J1958.1+3053; FSR 0177)
0.75
UTI
0.79
CN
0.65
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Nm (P>50%)
194
Core radius and density
2.4 [pc], 3.2 [pc-2]
- CN 0.79 Rich
- Cdens 0.65 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Kronberger 52 is a rich, moderately dense object of very high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~8.30 kpc) differs significantly from the median photometric distance (~4.99 kpc).
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a small 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 | 299.538 | 30.88 | 0.12 | -2.629 | -4.865 | -13.446 |
| Almeida et al. | 2025 | 299.535 | 30.882 | â | â | â | â |
| Hunt & Reffert | 2024 | 299.539 | 30.879 | 0.126 | -2.637 | -4.868 | -13.255 |
| Cavallo et al. | 2024 | 299.534 | 30.874 | 0.125 | â | â | â |
| Hunt & Reffert | 2023 | 299.539 | 30.879 | 0.126 | -2.637 | -4.868 | -13.255 |
| Just et al. | 2023 | 299.528 | 30.88 | â | â | â | â |
| Jadhav & Subramaniam | 2021 | 299.536 | 30.883 | â | â | â | â |
| Dias et al. | 2021 | 299.535 | 30.882 | 0.093 | -2.634 | -4.821 | â |
| Cantat-Gaudin et al. | 2020 | 299.536 | 30.883 | 0.106 | -2.622 | -4.837 | â |
| Cantat-Gaudin & Anders | 2020 | 299.536 | 30.883 | 0.106 | -2.622 | -4.837 | â |
| Bica et al. | 2019 | 299.531 | 30.892 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 299.536 | 30.883 | 0.106 | -2.622 | -4.837 | â |
| Dias et al. | 2018 | â | â | â | -3.35 | -2.95 | â |
| Sampedro et al. | 2017 | 299.533 | 30.888 | â | -1.32 | -4.44 | â |
| Kharchenko et al. | 2016 | 299.528 | 30.88 | â | â | â | â |
| Tadross | 2014 | 299.533 | 30.888 | â | â | â | â |
| Dias et al. | 2014 | 299.533 | 30.888 | â | -0.88 | -3.8 | â |
| Kharchenko et al. | 2013 | 299.533 | 30.883 | â | -2.43 | -4.1 | â |
| Bukowiecki et al. | 2011 | 299.533 | 30.889 | â | â | â | â |
| Kronberger et al. | 2006 | 299.533 | 30.888 | â | â | â | â |
| Dias et al. | 2002 | 299.533 | 30.888 | â | -0.87 | -3.79 | 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 | 4.99 | 3.09 | 2.67 | 407 | -0.137 | 1169 | â | 1 |
| Almeida et al. | 2025 | 5.33 | 2.86 | â | 644 | â | 1249 | â | â |
| Hunt & Reffert | 2024 | 6.76 | 3.88 | 2.67 | 102 | â | 7679(1) | â | â |
| Cavallo et al. | 2024 | 4.51 | 3.73 | â | 324 | -0.350 | â | â | â |
| Hunt & Reffert | 2023 | 6.76 | 3.88 | 2.67 | 102 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1000 | â | 139 | â | â |
| Jadhav & Subramaniam | 2021 | 4.99 | 2.49 | â | 407 | â | 1169 | â | 1(1) |
| Dias et al. | 2021 | 5.33 | 2.86 | â | 644 | 0.076 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 4.99 | 2.49 | â | 407 | â | â | â | â |
| Kounkel et al. | 2020 | 4.76 | 2.94 | â | 324 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.41 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.41 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.73 | 3.09 | â | 1000 | â | â | â | â |
| Tadross | 2014 | 0.70 | 7.73 | â | 130 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.73 | 3.09 | â | 1000 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 503 | â | â |
| Bukowiecki et al. | 2011 | 3.80(1) | 2.37 | â | 631 | â | â | â | â |
| Dias et al. | 2002 | 0.70 | 7.73 | â | 129 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.14 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.14 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.0282, e_all=0.0709.