OC 0471

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0.43 UTI
0.0
CN
1.0
Cdens
0.62
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members) 4.0 [arcmin]
  • CN 0.0 Sparse
  • Cdens 1.0 Very dense
  • CC3 0.62 Intermediate quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

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OC 0471 is a sparse, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster, but with a large variance across recent sources for the age parameter (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.

Relatively close Moderate 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 – 125.537 -42.979 0.667 -4.365 5.206 64.594
Hunt & Reffert 2024 125.532 -42.992 0.671 -4.343 5.184 –
Cavallo et al. 2024 125.526 -42.993 0.67 – – –
Hunt & Reffert 2023 125.532 -42.992 0.671 -4.343 5.184 –
Hao et al. 2022 125.541 -42.983 0.673 -4.381 5.111 –

💡 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 – – – – – 91* – –
Cavallo et al. 2024 1.56 1.92 – 186 -0.610 – – –
Hunt & Reffert 2023 1.45 1.95 1.54 10 – – – –
Hao et al. 2022 – 3.24 – 10 0.051 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 430 84.0 125.54 -42.98 0.66 -4.37 5.15 64.59 0.06

💡 Note: The % column shows the percentage of members that OC 0471 shares with each listed object.

Visualization

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