OC 0446

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0.59 UTI
0.44
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.44 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0446 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a close 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 large 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 – 121.201 -39.198 1.125 -4.572 3.957 24.138
Hunt & Reffert 2024 121.194 -39.188 1.122 -4.588 3.993 23.126
Cavallo et al. 2024 121.237 -39.12 1.131 – – –
Hunt & Reffert 2023 121.194 -39.188 1.122 -4.588 3.993 23.126
Hao et al. 2022 121.182 -39.194 1.132 -4.491 3.895 –

💡 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 – – – – – 92* – –
Cavallo et al. 2024 0.86 1.02 – 4 -0.250 – – –
Hunt & Reffert 2023 0.84 0.82 1.38 9 – – – –
Hao et al. 2022 – 4.61 – 6 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 363 100.0 121.21 -39.16 1.12 -4.58 3.98 25.42 0.23

💡 Note: The % column shows the percentage of members that OC 0446 shares with each listed object.

Visualization

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