OC 0318

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0.00 UTI
0.0
CN
0.37
Cdens
0.5
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.37 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

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OC 0318 is a sparse, loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Moderate 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 – 93.806 19.036 0.505 -0.06 -1.27 20.077
Hao et al. 2022 93.789 19.046 0.53 -0.059 -1.283 –

💡 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 – 1.75 – 6 0.537 – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
IRAS 06117+1901 100.0 93.7 19.0 0.48 -0.07 -1.26 -5.1 0.56
FSR 0909 52.0 93.87 19.04 0.48 -0.04 -1.26 20.08 0.4

💡 Note: The % column shows the percentage of members that OC 0318 shares with each listed object.

Visualization

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