Juchert 19
(SAI 33)
0.67
UTI
0.76
CN
0.43
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
3.7 [arcmin]
- CN 0.76 Rich
- Cdens 0.43 Loose
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
Juchert 19 is a rich, 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, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is moderately studied in the literature.
Very distant
High extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 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 |
| 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 |
| 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 6.39 | 3.20 | â | 7 | â | 540 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1778* | 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 |
| 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 | 0.87 | â | 1995 | â | â | â | â |
| Dias et al. | 2002 | 1.34 | 0.87 | â | 1995 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.