OC 0011

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0.68 UTI
0.88
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.2 [arcmin]
  • CN 0.88 Rich
  • 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 0011 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, old cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction Very massive Near-solar metallicity Old

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 272.992 -22.964 0.614 0.46 0.81 12.11
Hunt & Reffert 2024 272.993 -22.971 0.615 0.473 0.794 11.477
Cavallo et al. 2024 272.982 -22.963 0.615 – – –
Hunt & Reffert 2023 272.993 -22.971 0.615 0.473 0.794 11.477
Hao et al. 2022 272.989 -22.971 0.611 0.452 0.806 11.413

💡 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 – – – – – 8978* – –
Cavallo et al. 2024 1.66 3.93 – 832 -0.030 – – –
Hunt & Reffert 2023 1.54 3.33 3.03 1387 – – – –
Hao et al. 2022 – 4.54 – 1259 0.274 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Theia 1927 0.9 273.02 -22.91 0.81 0.27 0.74 12.18 0.29

💡 Note: The % column shows the percentage of members that OC 0011 shares with each listed object.

Visualization

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