OC 0390

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0.23 UTI
0.0
CN
0.14
Cdens
0.5
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 10.2 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.14 Very loose
  • CC3 0.5 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
OC 0390 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 112.783 -13.668 0.533 -1.186 0.242 26.972
Hunt & Reffert 2024 112.771 -13.626 0.548 -1.157 0.221 26.97
Cavallo et al. 2024 112.773 -13.645 0.538 – – –
Hunt & Reffert 2023 112.771 -13.626 0.548 -1.157 0.221 26.97
Hao et al. 2022 112.773 -13.664 0.534 -1.273 0.272 –

💡 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 – – – – – 106* – –
Cavallo et al. 2024 1.76 0.87 – 89 -0.140 – – –
Hunt & Reffert 2023 1.74 0.70 0.61 185 – – – –
Hao et al. 2022 – 1.01 – 316 0.051 – – –

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

Visualization

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