Kronberger 18
(MWSC 502; DSH J0518.6+3737)
0.38
UTI
0.3
CN
0.39
Cdens
0.12
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
4.0 [arcmin]
- CN 0.3 Poorly populated
- Cdens 0.39 Loose
- CC3 0.12 Very low quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
Kronberger 18 is a poorly populated, 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 moderately studied in the literature.
Note: This object shares a moderate percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
Moderate extinction
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 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 |
| Loktin & Popova | 2017 | 79.65 | 37.625 | â | -1.183 | -2.076 | â |
| Kharchenko et al. | 2016 | 79.663 | 37.631 | 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 |
| 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 18 | â | 127 | â | â |
| Loktin & Popova | 2017 | 2.62 | 1.17 | â | 513 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.70 | 2.17 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.70 | 2.17 | â | 18 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.70 | 2.17 | â | 18 | â | â | â | â |
| Dias et al. | 2002 | 3.25 | 4.00 | â | 100 | â | â | â | â |
