UBC 127

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0.20 UTI
0.84
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.39
Cdup
Radius (P>50% members) 3.8 [arcmin]
  • CN 0.84 Rich
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.0 Rarely studied
  • Cdup 0.39 Possibly duplicate

Overview

â„šī¸
UBC 127 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.

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 – 296.389 21.154 0.449 -0.369 -3.571 -18.114
Castro-Ginard et al. 2020 296.384 21.157 0.436 -0.35 -3.551 –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
FoF 321 60.7 296.39 21.15 0.45 -0.36 -3.57 -18.19 0.73
OC 0085 12.0 296.4 21.17 0.46 -0.38 -3.54 -18.05 0.0

💡 Note: The % column shows the percentage of members that UBC 127 shares with each listed object.

Visualization

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