Kronberger 13
(MWSC 3116; DSH J1925.2+1356)
0.72
UTI
0.56
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Stellar density (N50/rad)
28.5 [N/pc2]
- CN 0.56 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Kronberger 13 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.41 kpc) differs significantly from the median photometric distance (~1.46 kpc).
Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 291.314 | 13.946 | 0.293 | -1.796 | -4.224 | 18.62 |
| Hunt & Reffert | 2024 | 291.311 | 13.948 | 0.305 | -1.792 | -4.246 | 52.438 |
| Cavallo et al. | 2024 | 291.317 | 13.945 | 0.305 | â | â | â |
| Hunt & Reffert | 2023 | 291.311 | 13.948 | 0.305 | -1.792 | -4.246 | 52.438 |
| Just et al. | 2023 | 291.309 | 13.946 | â | â | â | â |
| Bica et al. | 2019 | 291.315 | 13.947 | â | â | â | â |
| Kharchenko et al. | 2016 | 291.309 | 13.946 | â | â | â | â |
| Kharchenko et al. | 2013 | 291.315 | 13.948 | â | 0.78 | -3.74 | â |
| Morales et al. | 2013 | 291.312 | 13.946 | â | â | â | â |
| Bukowiecki et al. | 2011 | 291.312 | 13.947 | â | â | â | â |
| Kronberger et al. | 2006 | 291.312 | 13.946 | â | â | â | â |
| Dias et al. | 2002 | 291.312 | 13.945 | â | 1.65 | 4.07 | 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 | 1.46 | 3.915 | 1.92 | 335 | 0.670 | 374 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1704(1) | â | â |
| Cavallo et al. | 2024 | 3.22 | 4.79 | â | 7 | 0.670 | â | â | â |
| Hunt & Reffert | 2023 | 2.96 | 5.33 | 1.92 | 8 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 335 | â | 61 | â | â |
| Kharchenko et al. | 2016 | 1.46 | 3.71 | â | 335 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.46 | 3.71 | â | 335 | â | â | â | â |
| Morales et al. | 2013 | 1.38 | â | â | 400 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 374 | â | â |
| Bukowiecki et al. | 2011 | 4.07(1) | 4.12 | â | 13 | â | â | â | â |
| Dias et al. | 2002 | 1.38 | 3.50 | â | 398 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.
Cavallo et al. (2024)
Gold sample.