OC 0413

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0.00 UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.31
Clit
0.0
Cdup
Radius (P>50% members) 1.9 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.31 Poorly studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
OC 0413 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (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. See table with shared members information.

Distant Moderate extinction Near-solar metallicity Old

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 – 108.706 -26.245 0.271 -2.071 2.762 79.813
Hu & Soubiran 2025 108.692 -26.25 – – – –
Hunt & Reffert 2024 108.695 -26.247 0.27 -2.08 2.77 80.108
Cavallo et al. 2024 108.692 -26.25 0.27 – – –
Hunt & Reffert 2023 108.695 -26.247 0.27 -2.08 2.77 80.108
Hao et al. 2022 108.707 -26.234 0.319 -2.059 2.768 –

💡 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
Hu & Soubiran 2025 – – – – -0.200* – – –
Hunt & Reffert 2024 – – – – – 550* – –
Cavallo et al. 2024 3.13 0.96 – 1479 0.300 – – –
Hunt & Reffert 2023 3.47 1.08 1.74 1117 – – – –
Hao et al. 2022 – 1.75 – 1000 0.370 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 71 100.0 108.7 -26.25 0.27 -2.07 2.77 80.02 0.13
FoF 665 100.0 108.7 -26.25 0.27 -2.07 2.77 79.92 0.51

💡 Note: The % column shows the percentage of members that OC 0413 shares with each listed object.

Visualization

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