OC 0330

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0.37 UTI
0.3
CN
0.43
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 6.9 [arcmin]
  • CN 0.3 Poorly populated
  • Cdens 0.43 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0330 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above 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 metallicity parameter (see Parameters). It is poorly studied in the literature.

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

Relatively close Low 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 – 98.787 12.664 0.534 0.753 -2.803 2.096
Zhang et al. 2024 98.794 12.647 – – – –
Hunt & Reffert 2024 98.794 12.647 0.538 0.689 -2.658 2.099
Cavallo et al. 2024 98.775 12.703 0.537 – – –
Hunt & Reffert 2023 98.794 12.647 0.538 0.689 -2.658 2.099
Hao et al. 2022 98.76 12.648 0.532 0.772 -2.798 –

💡 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 – – – – -0.126* – – –
Hunt & Reffert 2024 – – – – – 173* – –
Cavallo et al. 2024 1.75 0.86 – 417 0.220 – – –
Hunt & Reffert 2023 1.72 0.75 0.35 284 – – – –
Hao et al. 2022 – 0.19 – 316 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 451 83.3 98.79 12.66 0.53 0.76 -2.8 2.1 0.02

💡 Note: The % column shows the percentage of members that OC 0330 shares with each listed object.

Visualization

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