OC 0123

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0.02 UTI
0.36
CN
0.98
Cdens
0.38
CC3
0.25
Clit
0.06
Cdup
Radius (P>50% members) 5.2 [arcmin]
  • CN 0.36 Poorly populated
  • Cdens 0.98 Very dense
  • CC3 0.38 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 0.06 Very likely duplicate

Overview

â„šī¸
OC 0123 is a poorly populated, very dense object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close High 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 – 306.353 40.849 0.559 -3.026 -4.732 -20.579
Hunt & Reffert 2024 306.356 40.895 0.547 -3.047 -4.733 -20.622
Cavallo et al. 2024 306.353 40.853 0.549 – – –
Hunt & Reffert 2023 306.356 40.895 0.547 -3.047 -4.733 -20.622
Hao et al. 2022 306.321 40.793 0.551 -3.005 -4.828 –

💡 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 – – – – – 280* – –
Cavallo et al. 2024 1.86 3.24 – 10 0.130 – – –
Hunt & Reffert 2023 1.74 3.17 2.39 11 – – – –
Hao et al. 2022 – 3.67 – 13 0.611 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 503 94.4 306.37 40.88 0.51 -3.06 -4.57 -13.11 0.55
OC 0124 44.4 306.41 40.91 0.51 -3.1 -4.18 45.72 0.07

💡 Note: The % column shows the percentage of members that OC 0123 shares with each listed object.

Visualization

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