UBC 309

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0.05 UTI
0.88
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.1
Cdup
Radius (P>50% members) 5.9 [arcmin]
  • CN 0.88 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.1 Likely duplicate

Overview

UBC 309 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near 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.

⚠️ 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

Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 238.115 -55.414 0.485 -1.064 -2.244 -21.971
Castro-Ginard et al. 2020 238.1 -55.408 0.462 -1.036 -2.239

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UFMG 3 90.4 238.12 -55.42 0.49 -1.06 -2.24 -22.35 0.62
FoF 1182 52.6 238.1 -55.42 0.49 -1.06 -2.24 -22.35 0.0
OC 0636 20.6 238.09 -55.42 0.5 -1.09 -2.22 -21.97 0.0

💡 Note: The % column shows the percentage of members that UBC 309 shares with each listed object.

Visualization

Galactocentric position diagram

💡 Note: How are the galactocentric plots generated? See FAQ.