UBC 211

Click to load Aladin Lite
0.10 UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.19
Cdup
Radius (P>50% members) 8.2 [arcmin]
  • CN 0.77 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.19 Likely duplicate

Overview

â„šī¸
UBC 211 is a rich, very dense object of 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 – 95.265 -3.458 0.674 -1.493 1.602 24.717
Castro-Ginard et al. 2020 95.26 -3.441 0.67 -1.49 1.624 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 658 80.6 95.27 -3.45 0.67 -1.48 1.6 23.58 0.78
CWWDL 3289 41.2 95.27 -3.46 0.67 -1.5 1.6 24.15 0.0

💡 Note: The % column shows the percentage of members that UBC 211 shares with each listed object.

Visualization

â„šī¸