UBC 288

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0.20 UTI
0.83
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.35
Cdup
Radius (P>50% members) 6.8 [arcmin]
  • CN 0.83 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.35 Possibly duplicate

Overview

â„šī¸
UBC 288 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above 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 possibly a duplicate object, which shares a significant 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 – 191.007 -58.095 0.527 -2.212 -1.257 -8.79
Castro-Ginard et al. 2020 190.972 -58.097 0.505 -2.184 -1.277 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 1994 65.2 191.02 -58.1 0.53 -2.2 -1.25 -8.8 0.8
CWWDL 3107 41.7 191.0 -58.09 0.53 -2.2 -1.25 -8.94 0.0

💡 Note: The % column shows the percentage of members that UBC 288 shares with each listed object.

Visualization

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