Juchert 10

(MCM 53; fsr 1686; SAI 121; MCM2005b 53; MWSC 2241; MWSC 2239; LS 167; La Serena 167)

Click to load Aladin Lite
0.72 UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.52
Clit
1.0
Cdup
N50 (P>50% members) 240
Stellar density (N50/rad) 33.1 [N/pc2]
C3 classification AB
  • CN 0.8 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.52 Moderately studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 MOCAMOCA 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
ℹī¸
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 moderately studied in the literature.

Cavallo et al. (2024)
Wood sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.08 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.08 (50th percentile).

Bica et al. (2019)
Web updates in DAML02, some were later removed (2003 to 2010).

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Mercer et al. (2005)
Cluster of stars. Detected using no magnitude cut. Detected in 2MASS catalog with our algorithm. Appears in 2MASS images.

Data
🔍 Search references for Juchert 10 in: SciX Simbad
ℹī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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 – – –
Hunt & Reffert 2023 220.062 -60.379 0.244 -5.012 -2.745 -65.813
Just et al. 2023 220.059 -60.37 – – – –
Cantat-Gaudin et al. 2020 220.049 -60.375 0.107 -4.915 -2.592 –
Cantat-Gaudin & Anders 2020 220.049 -60.375 0.107 -4.915 -2.592 –
Soubiran et al. 2018 220.049 -60.375 – – – -70.74
Bica et al. 2019 220.075 -60.37 – – – –
Cantat-Gaudin et al. 2018 220.049 -60.375 0.107 -4.915 -2.592 –
Sampedro et al. 2017 220.079 -60.381 -4.65 -5.4 – –
Kharchenko et al. 2016 220.059 -60.37 – – – –
Kharchenko et al. 2013 220.071 -60.372 – -2.62 -4.64 –
Morales et al. 2013 220.05 -60.379 – – – –
Glushkova et al. 2010 220.028 -60.387 – – – –
Froebrich et al. 2007 220.071 -60.372 – – – –
Mercer et al. 2005 220.035 -60.372 – – – –
Dias et al. 2002 220.079 -60.381 – – – –

💡 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 99999– 5.41 5.26 2.87 316 0.710 5352 – –
Hunt & Reffert 2024 – – – – – 4262(1) – –
Cavallo et al. 2024 5.47 4.82 – 302 0.710 – – –
Hunt & Reffert 2023 3.21 5.53 2.87 85 – – – –
Just et al. 2023 – – – 316 – 6442 – –
Kounkel et al. 2020 3.46 5.29 – 31 – – – –
Cantat-Gaudin & Anders 2020 7.36 – – – – – – –
Soubiran et al. 2018 7.36 – – – – – – –
Cantat-Gaudin et al. 2018 7.36 – – – – – – –
Kharchenko et al. 2016 5.41 5.26 – 316 – – – –
Kharchenko et al. 2013 5.41 5.26 – 316 – – – –
Morales et al. 2013 4.02 – – 891 – – – –
Glushkova et al. 2010 4.02 4.67 – 891 – – – –
Dias et al. 2002 3.20 6.50 – 794 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization
ℹī¸
Juchert 10 UCC
Juchert 10 HUNT23
Juchert 10 CANTAT20
Galactocentric position diagram