UBC 144

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0.07 UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.13
Cdup
Radius (P>50% members) 5.6 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.13 Likely duplicate

Overview

â„šī¸
UBC 144 is a rich, very dense object of 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 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

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 307.51 45.917 0.679 -1.205 -0.916 -11.767
Castro-Ginard et al. 2020 307.504 45.925 0.669 -1.235 -0.951 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2253 86.6 307.51 45.92 0.68 -1.21 -0.92 -18.93 0.72
CWWDL 12285 82.1 307.51 45.92 0.68 -1.21 -0.92 -14.97 0.01

💡 Note: The % column shows the percentage of members that UBC 144 shares with each listed object.

Visualization

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