OC 0479

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0.62 UTI
0.57
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 20.8 [arcmin]
  • CN 0.57 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0479 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near 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.

Very 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 – 119.704 -49.18 2.476 -5.381 8.249 19.614
Hunt & Reffert 2024 119.552 -49.198 2.472 -5.388 8.237 13.021
Cavallo et al. 2024 119.801 -49.123 2.473 – – –
Hunt & Reffert 2023 119.552 -49.198 2.472 -5.388 8.237 13.021
Hao et al. 2022 119.535 -49.235 2.476 -5.378 8.264 19.224

💡 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 – – – – – 51* – –
Cavallo et al. 2024 0.41 0.70 – 3 -0.370 – – –
Hunt & Reffert 2023 0.39 0.21 0.65 7 – – – –
Hao et al. 2022 – 1.90 – 10 0.457 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
OCSN 199 100.0 119.78 -49.16 2.47 -5.39 8.25 20.01 0.43

💡 Note: The % column shows the percentage of members that OC 0479 shares with each listed object.

Visualization

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