UBC 274

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0.27 UTI
0.81
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.48
Cdup
Radius (P>50% members) 12.3 [arcmin]
  • CN 0.81 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.48 Possibly duplicate

Overview

â„šī¸
UBC 274 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 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 – 156.256 -72.558 0.52 -6.883 1.455 -23.512
Castro-Ginard et al. 2020 156.194 -72.575 0.508 -6.882 1.445 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 5 52.4 156.14 -72.53 0.52 -6.88 1.47 -23.22 0.72
OC 0560 2.0 154.51 -72.17 0.52 -6.87 1.69 -22.78 0.05

💡 Note: The % column shows the percentage of members that UBC 274 shares with each listed object.

Visualization

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