COIN-Gaia 14

(COIN 14)

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0.67 UTI
0.29
CN
1.0
Cdens
0.5
CC3
0.79
Clit
1.0
Cdup
C3 classification BB
Number of members (P>50%) 29
Radius (P>50% members) 7.8 [arcmin]
  • CN 0.29 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.79 Well-studied
  • Cdup 1.0 Unique
đŸ“Ĩ Members 📊 Colab đŸ”Ŧ Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (Îą, δ) 🔍 Simbad (Îą, δ)

Overview
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COIN-Gaia 14 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.

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

Close Low extinction Near-solar metallicity Intermediate age

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

Cavallo et al. (2024)
Gold sample.

Data
🔍 Search references for COIN-Gaia 14 in: SciX Simbad
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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 77.688 39.204 1.038 1.29 -6.656 8.747
Li et al. 2025 77.696 39.195 1.043 1.331 -6.598 –
Almeida et al. 2025 77.686 39.205 – – – –
Alfonso et al. 2024 77.571 39.147 0.982 1.287 -6.664 –
Zhang et al. 2024 77.694 39.203 – – – –
Hunt & Reffert 2024 77.694 39.203 1.007 1.299 -6.637 4.233
Cavallo et al. 2024 77.665 39.218 1.014 – – –
Hunt & Reffert 2023 77.694 39.203 1.007 1.299 -6.637 4.233
He et al. 2022 77.636 39.215 1.041 1.29 -6.652 –
Dias et al. 2021 77.686 39.205 1.04 1.329 -6.569 –
Cantat-Gaudin et al. 2020 77.696 39.195 1.043 1.331 -6.598 –
Cantat-Gaudin & Anders 2020 77.696 39.195 1.043 1.331 -6.598 –
Monteiro & Dias 2019 77.696 39.195 – – – 2.333
Cantat-Gaudin et al. 2019 77.696 39.195 1.04 1.33 -6.57 –

💡 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
Li et al. 2025 0.89 0.61 – 387 0.045 – – –
Almeida et al. 2025 0.92 1.04 – 182 – 58 – –
Alfonso et al. 2024 0.94 0.62 – 365 -0.076 – – –
Zhang et al. 2024 – – – – -0.246* – – –
Hunt & Reffert 2024 – – – – – 132* – –
Cavallo et al. 2024 0.95 0.75 – 275 0.530 – – –
Hunt & Reffert 2023 0.94 0.71 0.94 179 – – – –
He et al. 2022 – 1.25 – 56 – – – –
Tarricq et al. 2022 0.92 – – 479 – – – –
Dias et al. 2021 0.92 1.04 – 182 -0.076 – – –
Cantat-Gaudin et al. 2020 0.94 0.62 – 427 – – – –
Cantat-Gaudin & Anders 2020 0.93 – – – – – – –
Monteiro & Dias 2019 1.04 1.23 – 72 0.031 – – –
Cantat-Gaudin et al. 2019 0.93 – – – – – – –

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14417 93.1 77.66 39.19 1.03 1.29 -6.66 9.24 0.03

💡 Note: The % column shows the percentage of members that COIN-Gaia 14 shares with each listed object.

Visualization
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COIN-Gaia 14 UCC
COIN-Gaia 14 HUNT23
COIN-Gaia 14 CANTAT20
Galactocentric position diagram