UBC 55

Click to load Aladin Lite
0.00 UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members) 10.4 [arcmin]
  • CN 0.68 Moderately populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.0 Very likely duplicate

Overview

â„šī¸
UBC 55 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, 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.

Close Moderate extinction Near-solar metallicity Young

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 66.347 46.124 1.105 -1.073 -2.614 -11.574
Alfonso et al. 2024 66.373 46.128 1.075 -1.068 -2.615 –
Cantat-Gaudin et al. 2020 66.364 46.122 1.079 -1.067 -2.604 –
Cantat-Gaudin & Anders 2020 66.364 46.122 1.079 -1.067 -2.604 –

💡 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
Alfonso et al. 2024 0.90 1.38 – 30 -0.117 – – –
Cantat-Gaudin et al. 2020 0.90 1.38 – 34 – – – –
Cantat-Gaudin & Anders 2020 0.90 – – – – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
FSR 0686 100.0 66.37 46.13 1.1 -1.09 -2.61 -13.09 0.8

💡 Note: The % column shows the percentage of members that UBC 55 shares with each listed object.

Visualization

â„šī¸