OC 0407

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0.49 UTI
0.31
CN
1.0
Cdens
0.5
CC3
0.31
Clit
1.0
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.31 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.31 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0407 is a poorly populated, very dense object of intermediate 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 (see Parameters). It is poorly studied in the literature.

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

Close Low 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 – 107.321 -25.187 1.599 -4.98 3.665 23.759
Wei et al. 2025 107.411 -25.187 1.621 -4.922 3.635 –
Hunt & Reffert 2024 107.37 -25.201 1.622 -4.992 3.635 22.983
Cavallo et al. 2024 107.428 -25.164 1.624 – – –
Hunt & Reffert 2023 107.37 -25.201 1.622 -4.992 3.635 22.983
Hao et al. 2022 107.411 -25.222 1.586 -4.809 3.591 –

💡 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
Wei et al. 2025 0.71 0.47 – 15 0.000 202 0.44 –
Hunt & Reffert 2024 – – – – – 101* – –
Cavallo et al. 2024 0.69 0.44 – 14 -0.110 – – –
Hunt & Reffert 2023 0.60 0.12 0.53 25 – – – –
Hao et al. 2022 – 0.05 – 20 0.323 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 1204 77.4 107.41 -25.2 1.61 -4.99 3.63 24.02 0.03

💡 Note: The % column shows the percentage of members that OC 0407 shares with each listed object.

Visualization

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