OC 0266

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0.50 UTI
0.49
CN
1.0
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.6 [arcmin]
  • CN 0.49 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0266 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, 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.

Relatively close High extinction Massive 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 – 51.168 54.9 0.43 0.287 -1.02 19.573
Hunt & Reffert 2024 51.207 54.942 0.424 0.299 -0.99 17.312
Cavallo et al. 2024 51.092 54.909 0.426 – – –
Hunt & Reffert 2023 51.207 54.942 0.424 0.299 -0.99 17.312
Hao et al. 2022 51.117 54.893 0.443 0.331 -1.035 -26.659

💡 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 – – – – – 1013* – –
Cavallo et al. 2024 2.40 3.64 – 49 0.440 – – –
Hunt & Reffert 2023 2.16 3.60 2.47 68 – – – –
Hao et al. 2022 – 4.13 – 126 0.457 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 483 77.6 51.13 54.87 0.43 0.36 -1.08 -26.59 0.08

💡 Note: The % column shows the percentage of members that OC 0266 shares with each listed object.

Visualization

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