COIN-Gaia 33

(COIN 33)

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0.60 UTI
0.45
CN
0.82
Cdens
0.75
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members) 1.8 [arcmin]
  • CN 0.45 Poorly populated
  • Cdens 0.82 Dense
  • CC3 0.75 High quality
  • Clit 0.5 Moderately studied
  • Cdup 1.0 Unique

Overview

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COIN-Gaia 33 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a large distance, near 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 age and metallicity parameters (see Parameters). It is moderately studied in the literature.
Very distant Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 30.29 61.474 0.158 -1.339 -0.136 –
Li et al. 2025 30.276 61.475 0.123 -1.307 -0.071 –
Hunt & Reffert 2024 30.302 61.477 0.176 -1.339 -0.13 –
Cavallo et al. 2024 30.33 61.48 0.174 – – –
Hunt & Reffert 2023 30.302 61.477 0.176 -1.339 -0.13 –
Cantat-Gaudin et al. 2020 30.276 61.475 0.123 -1.307 -0.071 –
Cantat-Gaudin & Anders 2020 30.276 61.475 0.123 -1.307 -0.071 –
Monteiro & Dias 2019 30.276 61.475 – – – 3.391
Cantat-Gaudin et al. 2019 30.276 61.475 0.12 -1.31 -0.08 –

💡 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 3.09 2.19 – 557 -0.140 – – –
Hunt & Reffert 2024 – – – – – 711* – –
Cavallo et al. 2024 3.52 3.00 – 158 0.160 – – –
Hunt & Reffert 2023 5.20 3.21 1.51 61 – – – –
Cantat-Gaudin & Anders 2020 6.58 – – – – – – –
Monteiro & Dias 2019 10.49 2.29 – 6 0.042 – – –
Cantat-Gaudin et al. 2019 6.58 – – – – – – –

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

Visualization

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