Kronberger 12
(MWSC 808; DSH J0614.2+2229)
0.52
UTI
0.45
CN
1.0
Cdens
0.5
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
45
Core radius and density
0.9 [pc], 8.0 [pc-2]
- CN 0.45 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Kronberger 12 is a poorly populated, very dense object of intermediate 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 parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~3.66 kpc) differs significantly from the median photometric distance (~1.89 kpc).
Note: This object shares a significant 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 | 93.567 | 22.494 | 0.274 | -0.251 | -1.201 | â |
| Dias et al. | 2026 | 93.563 | 22.497 | 0.268 | -0.102 | -1.249 | 28.844 |
| Just et al. | 2023 | 93.553 | 22.484 | â | â | â | â |
| Bica et al. | 2019 | 93.565 | 22.501 | â | â | â | â |
| Dib et al. | 2018 | 93.562 | 22.483 | â | â | â | â |
| Sampedro et al. | 2017 | 93.562 | 22.498 | â | 1.35 | -1.45 | â |
| Kharchenko et al. | 2016 | 93.553 | 22.484 | â | â | â | â |
| Tadross | 2014 | 93.567 | 22.498 | â | â | â | â |
| Kharchenko et al. | 2013 | 93.562 | 22.483 | â | -1.04 | -5.85 | â |
| Bukowiecki et al. | 2011 | 93.567 | 22.5 | â | â | â | â |
| Kronberger et al. | 2006 | 93.565 | 22.498 | â | â | â | â |
| Dias et al. | 2002 | 93.562 | 22.498 | â | 13.28 | -0.72 | 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 | 1.89 | 2.615 | â | 474 | -0.222 | 202 | â | â |
| Dias et al. | 2026 | 3.11 | 2.45 | â | 207 | -0.222 | â | â | â |
| Just et al. | 2023 | â | â | â | 741 | â | 49 | â | â |
| Dib et al. | 2018 | 1.89 | â | â | 741 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.89 | 2.10 | â | 741 | â | â | â | â |
| Tadross | 2014 | 1.77 | 3.06 | â | 160 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.89 | 2.10 | â | 741 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 356 | â | â |
| Bukowiecki et al. | 2011 | 2.70(1) | 2.78 | â | 22 | â | â | â | â |
| Dias et al. | 2002 | 1.77 | 3.06 | â | 158 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010). The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.