OC 0237

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0.55 UTI
0.53
CN
0.7
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.53 Moderately populated
  • Cdens 0.7 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0237 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate distance, near 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 small percentage of members with 2 later reported entries. See table with shared members information.

Distant 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 – 22.672 62.405 0.335 -1.592 -0.418 –
Hunt & Reffert 2024 22.663 62.413 0.342 -1.595 -0.407 –
Cavallo et al. 2024 22.643 62.419 0.341 – – –
Hunt & Reffert 2023 22.663 62.413 0.342 -1.595 -0.407 –
Hao et al. 2022 22.71 62.361 0.329 -1.581 -0.447 –

💡 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 – – – – – 866* – –
Cavallo et al. 2024 3.42 2.13 – 19 0.320 – – –
Hunt & Reffert 2023 2.70 2.10 2.31 22 – – – –
Hao et al. 2022 – 4.08 – 13 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1993 25.0 22.91 62.39 0.32 -1.56 -0.37 – 0.08
CWWDL 10556 5.4 22.44 62.62 0.35 -1.52 -0.4 – 0.08

💡 Note: The % column shows the percentage of members that OC 0237 shares with each listed object.

Visualization

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