UBC 318

Click to load Aladin Lite
0.09 UTI
0.0
CN
0.07
Cdens
1.0
CC3
0.0
Clit
0.44
Cdup
Radius (P>50% members) 9.5 [arcmin]
  • CN 0.0 Sparse
  • Cdens 0.07 Very loose
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.44 Possibly duplicate

Overview

â„šī¸
UBC 318 is a sparse, very loose object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, very young cluster (see Parameters). It is rarely studied in the literature.

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

Relatively close Moderate extinction Massive Very young

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 251.118 -47.582 0.345 -0.945 -2.225 -43.355
Celli et al. 2024 251.144 -47.577 – – – –
Cantat-Gaudin et al. 2020 251.144 -47.577 0.329 -0.928 -2.223 –
Castro-Ginard et al. 2020 251.178 -47.587 0.33 -0.923 -2.214 –

💡 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
Celli et al. 2024 – – – 11 – 1944 – –
Cantat-Gaudin et al. 2020 2.79 1.83 – 11 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
Collinder 311 56.0 251.02 -47.47 0.35 -0.97 -2.29 -43.36 0.92
Hogg 21 40.0 251.41 -47.74 0.37 -0.97 -2.17 -43.91 0.95

💡 Note: The % column shows the percentage of members that UBC 318 shares with each listed object.

Visualization

â„šī¸