UBC 311

Click to load Aladin Lite
0.12 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.23
Cdup
Radius (P>50% members) 6.1 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.23 Likely duplicate

Overview

â„šī¸
UBC 311 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane. No fundamental parameter values are available for this object. It is rarely studied in the literature, with no articles listed in the last 6 years.

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.

No fundamental parameters

Castro-Ginard et al. (2020)
Coincidence with Sim et al. (2019, J. Korean Astron. Soc., 52, 145) or Liu & Pang (2019ApJS..245...32L), see Sect. 4.1.5.

Data

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 247.195 -54.964 0.712 0.018 -1.259 -3.258
Castro-Ginard et al. 2020 247.205 -54.971 0.692 0.047 -1.271 –

💡 Note: The UCC values are estimated from its identified members.

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2210 77.4 247.2 -54.96 0.71 0.02 -1.27 0.09 0.77
CWWDL 3733 58.9 247.18 -54.95 0.71 0.02 -1.25 -3.26 0.0

💡 Note: The % column shows the percentage of members that UBC 311 shares with each listed object.

Visualization

â„šī¸