OC 0185

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0.29 UTI
0.0
CN
0.32
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 12.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.32 Loose
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0185 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

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

Close Moderate extinction Near-solar metallicity Very young

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 – 332.684 63.302 1.085 -0.922 -2.259 -18.299
Hunt & Reffert 2024 332.741 63.396 1.077 -1.301 -2.486 -20.228
Cavallo et al. 2024 331.315 62.668 1.078 – – –
Hunt & Reffert 2023 332.741 63.396 1.077 -1.301 -2.486 -20.228
Hao et al. 2022 332.756 63.382 1.119 -0.739 -2.242 –

💡 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
Hunt & Reffert 2024 – – – – – 125* – –
Cavallo et al. 2024 0.92 1.31 – 5 -0.140 – – –
Hunt & Reffert 2023 0.90 1.12 2.27 6 – – – –
Hao et al. 2022 – 0.91 – 5 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1115 68.0 332.64 63.4 1.09 -0.89 -2.05 -23.53 0.42

💡 Note: The % column shows the percentage of members that OC 0185 shares with each listed object.

Visualization

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