OC 0310

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0.29 UTI
0.0
CN
0.45
Cdens
0.38
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 6.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.45 Loose
  • CC3 0.38 Low quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0310 is a sparse, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close Moderate extinction Near-solar metallicity 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 – 93.826 22.25 0.547 0.28 -1.872 –
Zhang et al. 2024 93.828 22.268 – – – –
Hunt & Reffert 2024 93.828 22.268 0.533 0.28 -1.825 –
Cavallo et al. 2024 93.815 22.348 0.53 – – –
Hunt & Reffert 2023 93.828 22.268 0.533 0.28 -1.825 –
Hao et al. 2022 93.808 22.259 0.549 0.27 -1.889 36.162

💡 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
Zhang et al. 2024 – – – – -0.141* – – –
Hunt & Reffert 2024 – – – – – 148* – –
Cavallo et al. 2024 1.97 1.83 – 26 -0.160 – – –
Hunt & Reffert 2023 1.88 1.93 0.71 21 – – – –
Hao et al. 2022 – 2.54 – 16 0.274 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 14036 48.0 93.87 22.3 0.54 0.24 -1.8 – 0.05

💡 Note: The % column shows the percentage of members that OC 0310 shares with each listed object.

Visualization

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