Juchert 13
(MWSC 1992; DSH J1201.6-6406; FSR 1600)
0.87
UTI
0.86
CN
1.0
Cdens
1.0
CC3
0.74
Clit
1.0
Cdup
Stellar density (N50/rad)
46.4 [N/pc2]
- CN 0.86 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.74 Moderately studied
- Cdup 1.0 Unique
Overview
Juchert 13 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age, metallicity, and mass parameters (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Note: This object shares a moderate 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 | 99999β | 180.43 | -64.099 | 0.305 | -8.162 | 0.261 | -5.957 |
| Li et al. | 2025 | 180.431 | -64.099 | 0.274 | -8.127 | 0.249 | β |
| Hu & Soubiran | 2025 | 180.419 | -64.097 | β | β | β | β |
| Almeida et al. | 2025 | 180.425 | -64.099 | β | β | β | β |
| Hunt & Reffert | 2024 | 180.434 | -64.101 | 0.316 | -8.163 | 0.266 | -6.105 |
| Cavallo et al. | 2024 | 180.419 | -64.097 | 0.315 | β | β | β |
| Hunt & Reffert | 2023 | 180.434 | -64.101 | 0.316 | -8.163 | 0.266 | -6.105 |
| Angelo et al. | 2023 | 180.396 | -64.094 | β | -8.16 | 0.29 | β |
| Just et al. | 2023 | 180.411 | -64.097 | β | β | β | β |
| Jadhav & Subramaniam | 2021 | 180.431 | -64.099 | β | β | β | β |
| Dias et al. | 2021 | 180.425 | -64.099 | 0.272 | -8.138 | 0.246 | -6.596 |
| Cantat-Gaudin et al. | 2020 | 180.431 | -64.099 | 0.274 | -8.127 | 0.249 | β |
| SΓ‘nchez et al. | 2020 | 180.421 | -64.1 | β | -8.185 | 0.328 | β |
| Cantat-Gaudin & Anders | 2020 | 180.431 | -64.099 | 0.274 | -8.127 | 0.249 | β |
| Soubiran et al. | 2018 | 180.431 | -64.099 | β | β | β | -6.6 |
| Bica et al. | 2019 | 180.42 | -64.099 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 180.431 | -64.099 | 0.274 | -8.127 | 0.249 | β |
| Sampedro et al. | 2017 | 180.421 | -64.1 | -4.84 | -0.83 | β | β |
| Kharchenko et al. | 2016 | 180.411 | -64.097 | β | β | β | β |
| Dias et al. | 2014 | 180.421 | -64.1 | β | -5.36 | -0.08 | β |
| Kharchenko et al. | 2013 | 180.42 | -64.1 | β | -15.39 | -5.77 | β |
| Bukowiecki et al. | 2011 | 180.404 | -64.098 | β | β | β | β |
| Kronberger et al. | 2006 | 180.423 | -64.1 | β | β | β | β |
| Dias et al. | 2002 | 180.421 | -64.1 | β | -5.36 | -0.08 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 2.895 | 2.3 | 1.96 | 1268 | -0.064 | 1130 | β | 4 |
| Li et al. | 2025 | 2.75 | 2.52 | β | 1439 | -0.064 | β | β | β |
| Hu & Soubiran | 2025 | β | β | β | β | -0.160(5) | β | β | β |
| Almeida et al. | 2025 | 2.62 | 1.78 | β | 3828 | β | 1654 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 3604(1) | β | β |
| Cavallo et al. | 2024 | 2.44 | 2.43 | β | 1995 | -0.110 | β | β | β |
| Hunt & Reffert | 2023 | 2.85 | 2.21 | 1.96 | 1084 | β | β | β | β |
| Angelo et al. | 2023 | 2.75 | 2.62 | β | 1413 | -0.060 | 12(1) | β | β |
| Just et al. | 2023 | β | β | β | 1000 | β | 472 | β | β |
| Jadhav & Subramaniam | 2021 | 3.39 | 1.74 | β | 2291 | β | 3562 | β | 4(1) |
| Dias et al. | 2021 | 2.62 | 1.78 | β | 3828 | 0.141 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.39 | 1.74 | β | 2291 | β | β | β | β |
| Kounkel et al. | 2020 | 3.28 | 2.41 | β | 832 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.29 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.29 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.29 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.79 | 2.63 | β | 1000 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.79 | 2.63 | β | 1000 | β | β | β | β |
| Bukowiecki et al. | 2012 | β | β | β | β | β | 606 | β | β |
| Bukowiecki et al. | 2011 | 2.97(1) | 2.24 | β | 1122 | β | β | β | β |
| Dias et al. | 2002 | 2.94 | 2.30 | β | 1122 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: worst fit. Isochrone match: intermediate fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.17 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.17 (50th percentile).
Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).