Skiff J0614+12.9

(FSR 0963; MWSC 817; Luginbuhl-Skiff 1; MWSC 818)

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0.85 UTI
0.76
CN
1.0
Cdens
0.5
CC3
1.0
Clit
1.0
Cdup
C3 classification BB
Number of members (P>50%) 119
Radius (P>50% members) 2.8 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 1.0 Very well-studied
  • Cdup 1.0 Unique
📥 Members 📊 Colab 🔬 Bayestar19 🔍 SciX 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview
Skiff J0614+12.9 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is very well-studied in the literature.

Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025): Mass determination: good fit. Isochrone match: good fit.

Cavallo et al. (2024): Gold sample.

Data
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 93.694 12.869 0.271 0.902 -1.977 45.64
Almeida et al. 2025 93.686 12.867 – – – –
Zhang et al. 2024 93.697 12.869 – – – –
Hunt & Reffert 2024 93.697 12.869 0.272 0.911 -1.976 42.68
Cavallo et al. 2024 93.684 12.871 0.27 – – –
Hunt & Reffert 2023 93.697 12.869 0.272 0.911 -1.976 42.68
Just et al. 2023 93.7 12.866 – – – –
Dias et al. 2021 93.686 12.867 0.257 0.918 -1.965 45.309
Cantat-Gaudin et al. 2020 93.691 12.87 0.249 0.915 -1.956 –
Soubiran et al. 2018 93.691 12.87 – – – 45.77
Bica et al. 2019 93.701 12.878 – – – –
Cantat-Gaudin et al. 2018 93.691 12.87 0.249 0.915 -1.956 –
Loktin & Popova 2017 93.705 12.872 – -0.31 -2.57 –
Kharchenko et al. 2016 93.7 12.866 – – – –
Kharchenko et al. 2013 93.708 12.865 – -1.22 -1.94 –
Froebrich et al. 2007 93.713 12.859 – – – –
Dias et al. 2002 93.696 12.871 – -0.31 -2.57 –

💡 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 2.95 1.93 – 342 – 370 – –
Zhang et al. 2024 – – – – 0.031* – – –
Hunt & Reffert 2024 – – – – – 651* – –
Cavallo et al. 2024 2.92 1.85 – 288 0.190 – – –
Hunt & Reffert 2023 3.36 1.69 0.96 247 – – – –
Just et al. 2023 – – – 282 – 29 – –
Dias et al. 2021 2.95 1.93 – 342 -0.193 – – –
Cantat-Gaudin et al. 2020 3.50 1.31 – 302 – – – –
Soubiran et al. 2018 3.60 – – – – – – –
Cantat-Gaudin et al. 2018 3.60 – – – – – – –
Loktin & Popova 2017 3.13 1.74 – 132 – – – –
Kharchenko et al. 2016 2.87 2.00 – 282 – – – –
Kharchenko et al. 2013 2.87 2.00 – 282 – – – –
Dias et al. 2002 3.15 1.77 – 251 – – – –

💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
(*): indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
LP 32 26.9 93.71 12.86 0.26 0.92 -1.98 45.64 0.01

💡 Note: The % column shows the percentage of members that Skiff J0614+12.9 shares with each listed object.

Visualization
Skiff J0614+12.9 UCC
Skiff J0614+12.9 HUNT23
Skiff J0614+12.9 CANTAT20
Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.