Kronberger 81
(MWSC 3511; DSH J2126.1+5331; FSR 0313)
0.85
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
11.7 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
Kronberger 81 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by very high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 321.54 | 53.527 | 0.177 | -2.547 | -3.283 | -34.37 |
| Hu & Soubiran | 2025 | 321.567 | 53.544 | â | â | â | â |
| Hunt & Reffert | 2024 | 321.539 | 53.53 | 0.141 | -2.477 | -3.218 | -36.965 |
| Cavallo et al. | 2024 | 321.566 | 53.544 | 0.15 | â | â | â |
| Hunt & Reffert | 2023 | 321.539 | 53.53 | 0.141 | -2.477 | -3.218 | -36.965 |
| Just et al. | 2023 | 321.539 | 53.531 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 321.547 | 53.534 | 0.228 | -2.61 | -3.324 | â |
| Cantat-Gaudin & Anders | 2020 | 321.547 | 53.534 | 0.228 | -2.61 | -3.324 | â |
| Soubiran et al. | 2018 | 321.547 | 53.534 | â | â | â | -85.4 |
| Bica et al. | 2019 | 321.542 | 53.535 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 321.547 | 53.534 | 0.228 | -2.61 | -3.324 | â |
| Loktin & Popova | 2017 | 321.54 | 53.531 | â | -0.52 | -0.554 | â |
| Kharchenko et al. | 2016 | 321.539 | 53.531 | â | â | â | â |
| Dias et al. | 2014 | 321.538 | 53.533 | â | 0.06 | -1.82 | â |
| Kharchenko et al. | 2013 | 321.544 | 53.534 | â | -1.63 | -0.97 | â |
| Kharchenko et al. | 2012 | 321.544 | 53.534 | â | -1.63 | -0.97 | â |
| Kronberger et al. | 2006 | 321.537 | 53.533 | â | â | â | â |
| Dias et al. | 2002 | 321.538 | 53.533 | â | 0.06 | -1.82 | 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 | 5.24 | 5.385 | 2.5 | 398 | -0.195 | 2012 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.490(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2432(1) | â | â |
| Cavallo et al. | 2024 | 4.06 | 4.71 | â | 1288 | 0.100 | â | â | â |
| Hunt & Reffert | 2023 | 5.24 | 5.19 | 2.50 | 401 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 1592 | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.90 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.90 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.49 | 2.43 | â | 692 | â | â | â | â |
| Kharchenko et al. | 2016 | 7.50 | 5.58 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 7.50 | 5.58 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2012 | 7.50 | 5.58 | â | 398 | â | â | â | â |
| Kronberger et al. | 2006 | 5.90 | 4.65 | â | â | â | â | â | â |
| Dias et al. | 2002 | 7.50 | 5.58 | â | 398 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.