Kronberger 73
(MWSC 3287; DSH J2013.7+3644; FSR 0203)
0.74
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.6
Clit
1.0
Cdup
Stellar density (N50/rad)
11.3 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.6 Moderately studied
- Cdup 1.0 Unique
Overview
Kronberger 73 is a rich, very dense object of high C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-poor, 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 (~7.41 kpc) differs significantly from the median photometric distance (~2.94 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 | 303.438 | 36.75 | 0.135 | -3.576 | -5.666 | -38.71 |
| Hunt & Reffert | 2024 | 303.439 | 36.746 | 0.135 | -3.58 | -5.652 | -34.458 |
| Cavallo et al. | 2024 | 303.428 | 36.758 | 0.135 | â | â | â |
| Hunt & Reffert | 2023 | 303.439 | 36.746 | 0.135 | -3.58 | -5.652 | -34.458 |
| Just et al. | 2023 | 303.437 | 36.746 | â | â | â | â |
| Bica et al. | 2019 | 303.453 | 36.749 | â | â | â | â |
| Kharchenko et al. | 2016 | 303.437 | 36.746 | â | â | â | â |
| Kharchenko et al. | 2013 | 303.442 | 36.749 | â | -3.99 | -1.91 | â |
| Bukowiecki et al. | 2011 | 303.442 | 36.754 | â | â | â | â |
| Kronberger et al. | 2006 | 303.447 | 36.749 | â | â | â | â |
| Dias et al. | 2002 | 303.446 | 36.749 | â | -0.93 | 0.54 | 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 | 2.935 | 3.42 | 2.64 | 676 | -0.520 | 2130 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2130(1) | â | â |
| Cavallo et al. | 2024 | 5.04 | 4.80 | â | 138 | -0.520 | â | â | â |
| Hunt & Reffert | 2023 | 6.26 | 4.78 | 2.64 | 56 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 676 | â | 22 | â | â |
| Kharchenko et al. | 2016 | 2.69 | 3.42 | â | 676 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.69 | 3.42 | â | 676 | â | â | â | â |
| Bukowiecki et al. | 2012 | â | â | â | â | â | 4031 | â | â |
| Bukowiecki et al. | 2011 | 3.18(1) | 1.98 | â | 1585 | â | â | â | â |
| Dias et al. | 2002 | 1.70 | 3.01 | 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)
Silver sample.