Juchert 19
(SAI 33)
0.49
UTI
0.76
CN
0.11
Cdens
0.75
CC3
0.42
Clit
1.0
Cdup
Nm (P>50%)
117
Core radius and density
4.0 [pc], 0.6 [pc-2]
- CN 0.76 Rich
- Cdens 0.11 Very loose
- CC3 0.75 High quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
Juchert 19 is a rich, very loose object of high C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 60.572 | 52.44 | 0.146 | -0.207 | 0.153 | -39.727 |
| Almeida et al. | 2025 | 60.583 | 52.448 | â | â | â | â |
| Hunt & Reffert | 2024 | 60.582 | 52.444 | 0.156 | -0.226 | 0.16 | -39.727 |
| Celli et al. | 2024 | 60.585 | 52.446 | â | â | â | â |
| Cavallo et al. | 2024 | 60.547 | 52.435 | 0.149 | â | â | â |
| Hunt & Reffert | 2023 | 60.582 | 52.444 | 0.156 | -0.226 | 0.16 | -39.727 |
| Dias et al. | 2021 | 60.583 | 52.448 | 0.114 | -0.184 | 0.185 | â |
| Cantat-Gaudin et al. | 2020 | 60.585 | 52.446 | 0.102 | -0.141 | 0.176 | â |
| Zhong et al. | 2020 | 60.585 | 52.446 | â | -0.141 | 0.176 | 348.841 |
| Cantat-Gaudin & Anders | 2020 | 60.585 | 52.446 | 0.102 | -0.141 | 0.176 | â |
| Cantat-Gaudin et al. | 2018 | 60.585 | 52.446 | 0.102 | -0.141 | 0.176 | â |
| Sampedro et al. | 2017 | 60.583 | 52.444 | â | -0.09 | 2.0 | â |
| Glushkova et al. | 2010 | 60.584 | 52.444 | â | â | â | â |
| Kronberger et al. | 2006 | 60.578 | 52.44 | â | â | â | â |
| Dias et al. | 2002 | 60.583 | 52.444 | â | -4.65 | -3.83 | 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 | 5.645 | 3.2 | 2.36 | 31 | 0.000 | 540 | â | â |
| Almeida et al. | 2025 | 6.39 | 3.20 | â | 7 | â | 540 | â | â |
| Hunt & Reffert | 2024 | 5.46 | 3.71 | 2.36 | 31 | â | 1778(1) | â | â |
| Celli et al. | 2024 | â | â | â | 8 | â | 215 | â | â |
| Cavallo et al. | 2024 | 3.91 | 3.23 | â | 54 | 0.710 | â | â | â |
| Hunt & Reffert | 2023 | 5.46 | 3.71 | 2.36 | 31 | â | â | â | â |
| Dias et al. | 2021 | 6.39 | 3.20 | â | 7 | -0.212 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 5.83 | 3.33 | â | 8 | â | â | â | â |
| Kounkel et al. | 2020 | 4.44 | 2.58 | â | 1122 | â | â | â | â |
| Zhong et al. | 2020 | 7.63(1) | â | â | â | 0.000 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 7.63 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 7.63 | â | â | â | â | â | â | â |
| Glushkova et al. | 2010 | 1.34 | 0.88 | â | 1995 | â | â | â | â |
| Dias et al. | 2002 | 1.34 | 0.88 | â | 1995 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.22 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.22 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.4151, e_all=0.2193.
Bica et al. (2019)
Asterisms and cluster alikes by B. Alessi reported in DAML02.