Kronberger 92
0.47
UTI
0.27
CN
0.94
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members)
6.6 [arcmin]
- CN 0.27 Poorly populated
- Cdens 0.94 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.31 Poorly studied
- Cdup 1.0 Unique
Overview
Kronberger 92 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 83.9 | 44.172 | 0.801 | 1.934 | -2.583 | -28.682 |
| Zhang et al. | 2024 | 83.852 | 44.195 | â | â | â | â |
| Hunt & Reffert | 2024 | 83.852 | 44.195 | 0.799 | 1.896 | -2.541 | -29.517 |
| Cavallo et al. | 2024 | 83.873 | 44.199 | 0.797 | â | â | â |
| Hunt & Reffert | 2023 | 83.852 | 44.195 | 0.799 | 1.896 | -2.541 | -29.517 |
| Bica et al. | 2019 | 83.831 | 44.166 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.156* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 74* | â | â |
| Cavallo et al. | 2024 | 1.22 | 0.58 | â | 295 | 0.400 | â | â | â |
| Hunt & Reffert | 2023 | 1.19 | 0.75 | 0.50 | 165 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.