Kronberger 28
(MWSC 3255; DSH J2006.5+3534)
0.16
UTI
0.0
CN
0.03
Cdens
0.12
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
16
Core radius and density
1.4 [pc], 0.2 [pc-2]
- CN 0.0 Sparse
- Cdens 0.03 Very loose
- CC3 0.12 Very low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
Kronberger 28 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~4.09 kpc) differs significantly from the median photometric distance (~2.69 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 301.656 | 35.57 | 0.245 | -3.208 | -5.611 | â |
| Hunt & Reffert | 2024 | 301.659 | 35.55 | 0.24 | -3.222 | -5.627 | â |
| Hunt & Reffert | 2023 | 301.659 | 35.55 | 0.24 | -3.222 | -5.627 | â |
| Just et al. | 2023 | 301.622 | 35.567 | â | â | â | â |
| Bica et al. | 2019 | 301.632 | 35.57 | â | â | â | â |
| Kharchenko et al. | 2016 | 301.622 | 35.567 | â | â | â | â |
| Tadross | 2014 | 301.633 | 35.576 | â | â | â | â |
| Dias et al. | 2014 | 301.633 | 35.576 | â | -3.54 | -5.8 | â |
| Kharchenko et al. | 2013 | 301.627 | 35.57 | â | -2.11 | -5.43 | â |
| Bukowiecki et al. | 2011 | 301.637 | 35.575 | â | â | â | â |
| Kronberger et al. | 2006 | 301.632 | 35.576 | â | â | â | â |
| Dias et al. | 2002 | 301.633 | 35.576 | â | -2.11 | -5.43 | 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 | 2.69 | 2.6 | 1.68 | 399 | â | 381 | â | â |
| Hunt & Reffert | 2024 | 3.77 | 2.60 | 1.68 | 190 | â | 381(1) | â | â |
| Hunt & Reffert | 2023 | 3.77 | 2.60 | 1.68 | 191 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 716 | â | 99 | â | â |
| Kharchenko et al. | 2016 | 2.69 | 2.43 | â | 716 | â | â | â | â |
| Tadross | 2014 | 0.55 | 7.13 | â | 400 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.69 | 2.43 | â | 716 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 845 | â | â |
| Bukowiecki et al. | 2011 | 2.28(1) | 2.84 | â | 28 | â | â | â | â |
| Dias et al. | 2002 | 0.55 | 7.13 | â | 398 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.36 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.36 (50th percentile).
Bica et al. (2019)
The Preliminary Amateur Open Cluster Catalog, Version 08/03/2003.