Juchert 10
(FSR 1686; SAI 121; MWSC 2241; MWSC 2239; LS 167; La Serena 167)
0.82
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
33.1 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
Juchert 10 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by very high extinction. It is catalogued as a very massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Note: This object shares a small 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 | 220.068 | -60.375 | 0.184 | -4.987 | -2.691 | -70.495 |
| Hunt & Reffert | 2024 | 220.062 | -60.379 | 0.244 | -5.012 | -2.745 | -65.813 |
| Cavallo et al. | 2024 | 220.049 | -60.377 | 0.25 | â | â | â |
| Hunt & Reffert | 2023 | 220.062 | -60.379 | 0.244 | -5.012 | -2.745 | -65.813 |
| Just et al. | 2023 | 220.059 | -60.37 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 220.049 | -60.375 | 0.107 | -4.915 | -2.592 | â |
| Cantat-Gaudin & Anders | 2020 | 220.049 | -60.375 | 0.107 | -4.915 | -2.592 | â |
| Soubiran et al. | 2018 | 220.049 | -60.375 | â | â | â | -70.74 |
| Bica et al. | 2019 | 220.075 | -60.37 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 220.049 | -60.375 | 0.107 | -4.915 | -2.592 | â |
| Kharchenko et al. | 2016 | 220.059 | -60.37 | â | â | â | â |
| Kharchenko et al. | 2013 | 220.071 | -60.372 | â | -2.62 | -4.64 | â |
| Glushkova et al. | 2010 | 220.028 | -60.387 | â | â | â | â |
| Froebrich et al. | 2007 | 220.071 | -60.372 | â | â | â | â |
| Dias et al. | 2002 | 220.079 | -60.381 | â | â | â | 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 | 5.41 | 5.16 | 2.87 | 316 | 0.710 | 5352 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 4262(1) | â | â |
| Cavallo et al. | 2024 | 5.47 | 4.82 | â | 302 | 0.710 | â | â | â |
| Hunt & Reffert | 2023 | 3.21 | 5.53 | 2.87 | 85 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 316 | â | 6442 | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.36 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 7.36 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.36 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.41 | 5.16 | â | 316 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.41 | 5.16 | â | 316 | â | â | â | â |
| Glushkova et al. | 2010 | 4.02 | 4.59 | â | 891 | â | â | â | â |
| Dias et al. | 2002 | 3.20 | 6.39 | â | 794 | 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)
Wood sample.