OC 0051

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0.04 UTI
0.0
CN
0.86
Cdens
0.75
CC3
0.0
Clit
0.12
Cdup
Radius (P>50% members) 3.9 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.86 Dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.12 Likely duplicate

Overview

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OC 0051 is a sparse, dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a metal-rich, very young cluster (see Parameters). It is rarely studied in the literature.

âš ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

High extinction Metal-rich Very young

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 280.819 -3.725 0.502 -0.65 -2.185 –
Hao et al. 2022 280.81 -3.731 0.514 -0.647 -2.186 –

💡 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
Hao et al. 2022 – 4.85 – 1 0.611 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 1764 92.0 280.83 -3.75 0.47 -0.63 -2.18 29.97 0.12
UBC 353 88.0 280.84 -3.74 0.46 -0.63 -2.19 29.97 0.68

💡 Note: The % column shows the percentage of members that OC 0051 shares with each listed object.

Visualization

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