Juchert 18
(MWSC 893)
0.35
UTI
0.0
CN
0.21
Cdens
0.25
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.21 Very loose
- CC3 0.25 Low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
Juchert 18 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is moderately studied in the literature.
Very distant
Moderate extinction
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 97.865 | 6.805 | 0.162 | -0.018 | -0.022 | 80.085 |
| Celli et al. | 2024 | 97.864 | 6.804 | β | β | β | β |
| Just et al. | 2023 | 97.855 | 6.805 | β | β | β | β |
| Cantat-Gaudin et al. | 2020 | 97.864 | 6.804 | 0.148 | 0.059 | 0.057 | β |
| SΓ‘nchez et al. | 2020 | 97.867 | 6.803 | β | -0.072 | -0.189 | β |
| Cantat-Gaudin & Anders | 2020 | 97.864 | 6.804 | 0.148 | 0.059 | 0.057 | β |
| Soubiran et al. | 2018 | 97.864 | 6.804 | β | β | β | 55.72 |
| Cantat-Gaudin et al. | 2018 | 97.864 | 6.804 | 0.148 | 0.059 | 0.057 | β |
| Kharchenko et al. | 2016 | 97.855 | 6.805 | β | β | β | β |
| Kharchenko et al. | 2013 | 97.863 | 6.804 | β | -1.81 | -2.04 | β |
| Kronberger et al. | 2006 | 97.865 | 6.803 | β | β | β | β |
| Dias et al. | 2002 | 97.867 | 6.803 | β | -1.81 | -2.04 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Celli et al. | 2024 | β | β | β | 24 | β | 213 | β | β |
| Just et al. | 2023 | β | β | β | 1047 | β | 146 | β | β |
| Cantat-Gaudin et al. | 2020 | 5.73 | 2.02 | β | 25 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 5.64 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 5.64 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 5.64 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.29 | 1.94 | β | 1047 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.29 | 1.94 | β | 1047 | β | β | β | β |
| Dias et al. | 2002 | 2.29 | 1.94 | β | 1047 | β | β | β | β |

