Kronberger 79
(MWSC 3138; DSH J1933.9+1831)
0.88
UTI
0.65
CN
1.0
Cdens
1.0
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
0.8 [arcmin]
- CN 0.65 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
Kronberger 79 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a large* distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~6.10 kpc) differs significantly from the median photometric distance (~3.37 kpc).
Distant
High 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 | 293.479 | 18.519 | 0.164 | -2.773 | -5.332 | â |
| Almeida et al. | 2025 | 293.477 | 18.521 | â | â | â | â |
| Hunt & Reffert | 2024 | 293.476 | 18.518 | 0.175 | -2.793 | -5.34 | â |
| Cavallo et al. | 2024 | 293.477 | 18.519 | 0.175 | â | â | â |
| Hunt & Reffert | 2023 | 293.476 | 18.518 | 0.175 | -2.793 | -5.34 | â |
| Just et al. | 2023 | 293.469 | 18.526 | â | â | â | â |
| Dias et al. | 2021 | 293.477 | 18.521 | 0.127 | -2.748 | -5.308 | â |
| Cantat-Gaudin et al. | 2020 | 293.478 | 18.522 | 0.148 | -2.718 | -5.33 | â |
| Cantat-Gaudin & Anders | 2020 | 293.478 | 18.522 | 0.148 | -2.718 | -5.33 | â |
| Bica et al. | 2019 | 293.478 | 18.522 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 293.478 | 18.522 | 0.148 | -2.718 | -5.33 | â |
| Loktin & Popova | 2017 | 293.475 | 18.526 | â | 1.705 | -4.25 | â |
| Kharchenko et al. | 2016 | 293.469 | 18.526 | â | â | â | â |
| Dias et al. | 2014 | 293.479 | 18.52 | â | -1.22 | -2.61 | â |
| Kharchenko et al. | 2013 | 293.475 | 18.528 | â | 3.03 | -3.09 | â |
| Kronberger et al. | 2006 | 293.479 | 18.52 | â | â | â | â |
| Dias et al. | 2002 | 293.479 | 18.52 | â | 3.03 | -3.09 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 3.30 | 4.14 | â | 6 | â | 621 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3745* | â | â |
| Cavallo et al. | 2024 | 4.29 | 4.76 | â | 10 | 0.750 | â | â | â |
| Hunt & Reffert | 2023 | 5.32 | 5.49 | 2.62 | 11 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 245 | â | 541 | â | â |
| Dias et al. | 2021 | 3.30 | 4.14 | â | 6 | 0.061 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.65 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.36 | 2.62 | â | 1047 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.37 | 4.45 | â | 245 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.37 | 4.45 | â | 245 | â | â | â | â |
| Kronberger et al. | 2006 | 3.60* | 4.71* | â | 25* | â | â | â | â |
| Dias et al. | 2002 | 2.70 | 4.03 | â | 224 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Silver sample.