OC 0124

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0.07 UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.12
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.58 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 0.12 Likely duplicate

Overview

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OC 0124 is a moderately populated, very dense object of high 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, young cluster (see Parameters). It is poorly studied in the literature.

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

Relatively close High extinction 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 – 306.406 40.908 0.511 -3.095 -4.179 45.724
Hunt & Reffert 2024 306.438 40.924 0.491 -3.115 -4.137 45.631
Cavallo et al. 2024 306.409 40.914 0.492 – – –
Hunt & Reffert 2023 306.438 40.924 0.491 -3.115 -4.137 45.631
Hao et al. 2022 306.448 40.911 0.546 -3.017 -4.558 –

💡 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 – – – – – 380* – –
Cavallo et al. 2024 1.36 3.06 – 123 -0.480 – – –
Hunt & Reffert 2023 1.90 3.04 2.18 64 – – – –
Hao et al. 2022 – 1.85 – 16 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 87.9 306.37 40.88 0.51 -3.06 -4.57 -13.11 0.55
OC 0123 24.2 306.35 40.85 0.56 -3.03 -4.73 -20.58 0.02

💡 Note: The % column shows the percentage of members that OC 0124 shares with each listed object.

Visualization

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