OC 0401

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0.51 UTI
0.36
CN
0.92
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 4.6 [N/pc2]
  • CN 0.36 Poorly populated
  • Cdens 0.92 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0401 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the absorption and metallicity parameters (see Parameters). It is poorly studied in the literature.

Note: This object shares a significant percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Liu et al. (2025)
Classified as primordial binary cluster 310 along with OC_0395.

Palma et al. (2025)
Classified as genetic pair P242, along with OC_0395.

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 104.85 -23.332 1.176 -3.121 3.387 37.181
Cavallo et al. 2024 104.927 -23.547 1.181 – – –
Hunt & Reffert 2023 104.686 -23.326 1.185 -3.069 3.395 35.587
Hao et al. 2022 104.713 -23.363 1.143 -2.989 3.346 –

💡 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] Bfrac BSS
UCC 99999– 0.81 0.335 0.53 12 0.141 – – –
Liu et al. 2025 0.77 0.02 – 28 – – – –
Cavallo et al. 2024 0.92 0.52 – 6 -0.330 – – –
Hunt & Reffert 2023 0.81 0.15 0.53 14 – – – –
Hao et al. 2022 – 1.92 – 10 0.611 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
OC 0399 58.3 104.93 -23.26 1.17 -3.12 3.36 37.18 0.31

💡 Note: The % column shows the percentage of members that OC 0401 shares with each listed object.

Visualization

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