UBC 140

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0.14 UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.0
Clit
0.25
Cdup
Radius (P>50% members) 7.1 [arcmin]
  • CN 0.76 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.0 Rarely studied
  • Cdup 0.25 Possibly duplicate

Overview

â„šī¸
UBC 140 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 – 305.369 38.6 0.561 -3.237 -5.996 -22.57
Castro-Ginard et al. 2020 305.375 38.6 0.551 -3.247 -5.985 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 2179 74.6 305.39 38.61 0.56 -3.25 -5.98 -22.57 0.55
CWWDL 2501 2.6 305.47 38.74 0.56 -3.28 -5.68 – 0.04
Collinder 422 0.9 305.93 38.5 0.56 -3.42 -5.79 -21.9 0.95

💡 Note: The % column shows the percentage of members that UBC 140 shares with each listed object.

Visualization

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