UBC 369

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0.19 UTI
0.62
CN
0.7
Cdens
1.0
CC3
0.0
Clit
0.41
Cdup
Radius (P>50% members) 7.7 [arcmin]
  • CN 0.62 Moderately populated
  • Cdens 0.7 Moderately dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.41 Possibly duplicate

Overview

â„šī¸
UBC 369 is a moderately populated, moderately dense object of very high C3 quality. Its parallax locates it at a moderate 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 – 303.576 36.702 0.483 -2.904 -5.703 -0.682
Castro-Ginard et al. 2020 303.543 36.733 0.483 -2.908 -5.692 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2178 58.7 303.58 36.71 0.48 -2.88 -5.7 3.46 0.23
Dolidze 3 36.0 303.82 36.83 0.49 -2.87 -5.63 -26.2 0.92

💡 Note: The % column shows the percentage of members that UBC 369 shares with each listed object.

Visualization

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