OC 0623

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0.41 UTI
0.28
CN
1.0
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members) 3.2 [arcmin]
  • CN 0.28 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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OC 0623 is a poorly populated, very dense object of high 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, very young cluster (see Parameters). It is rarely studied in the literature.

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Low extinction Near-solar metallicity 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 – 223.288 -54.099 0.907 -2.825 -2.302 -17.204
Hao et al. 2022 223.299 -54.108 0.896 -2.848 -2.287 –

💡 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 – 0.77 – 16 0.051 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 95 100.0 223.29 -54.1 0.91 -2.8 -2.3 -17.2 0.23
CWWDL 14468 100.0 223.29 -54.1 0.91 -2.81 -2.31 -17.2 0.0

💡 Note: The % column shows the percentage of members that OC 0623 shares with each listed object.

Visualization

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