Kronberger 18
(MWSC 502; DSH J0518.6+3737)
0.26
UTI
0.3
CN
0.08
Cdens
0.12
CC3
0.39
Clit
1.0
Cdup
Nm (P>50%)
30
Core radius and density
2.9 [pc], 0.4 [pc-2]
- CN 0.3 Poorly populated
- Cdens 0.08 Very loose
- CC3 0.12 Very low quality
- Clit 0.39 Poorly studied
- Cdup 1.0 Unique
Overview
Kronberger 18 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a very young cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a moderate percentage of members with 2 later reported entries. 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 | 79.597 | 37.61 | 0.295 | 0.075 | -0.237 | 11.396 |
| Just et al. | 2023 | 79.663 | 37.631 | â | â | â | â |
| Bica et al. | 2019 | 79.651 | 37.619 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | 2.01 | -3.89 | â |
| Loktin & Popova | 2017 | 79.65 | 37.625 | â | -1.183 | -2.076 | â |
| Sampedro et al. | 2017 | 79.65 | 37.625 | â | -24.3 | -11.25 | â |
| Kharchenko et al. | 2016 | 79.663 | 37.631 | â | â | â | â |
| Tadross | 2014 | 79.65 | 37.622 | â | â | â | â |
| Dias et al. | 2014 | 79.65 | 37.625 | â | -1.55 | -5.74 | â |
| Kharchenko et al. | 2013 | 79.672 | 37.63 | â | -4.29 | -6.7 | â |
| Kharchenko et al. | 2012 | 79.672 | 37.63 | â | -4.29 | -6.7 | â |
| Bukowiecki et al. | 2011 | 79.654 | 37.628 | â | â | â | â |
| Kronberger et al. | 2006 | 79.65 | 37.622 | â | â | â | â |
| Dias et al. | 2002 | 79.65 | 37.625 | â | -1.55 | -5.74 | 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 | 2.7 | 2.21 | â | 18 | â | 328 | â | â |
| Just et al. | 2023 | â | â | â | 18 | â | 127 | â | â |
| Loktin & Popova | 2017 | 2.62 | 1.19 | â | 513 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.70 | 2.21 | â | 18 | â | â | â | â |
| Tadross | 2014 | 3.25 | 4.07 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.70 | 2.21 | â | 18 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 530 | â | â |
| Kharchenko et al. | 2012 | 2.70 | 2.21 | â | 18 | â | â | â | â |
| Bukowiecki et al. | 2011 | 2.53(1) | 2.30 | â | 14 | â | â | â | â |
| Dias et al. | 2002 | 3.25 | 4.07 | â | 100 | 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.