UBC 385

Click to load Aladin Lite
C3
N_50
r_50
AA 35 6.7
Summary

UBC 385 is a poorly populated, very dense object of very high C3 quality. It is located at a close distance from the Sun, above the mid-plane. It is poorly studied in the literature.

Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Castro-Ginard et al. (2020) 317.945 60.077 1.18 -2.538 -3.466
Cantat-Gaudin et al. (2020) 317.94 60.092 1.178 -2.53 -3.468
He et al. (2022) 317.952 60.014 1.187 -2.521 -3.517
Celli et al. (2024) 317.94 60.092
Alfonso et al. (2024) 318.434 59.506 1.116 -2.553 -3.558
           
UCC 317.944 60.023 1.176 -2.531 -3.506 -17.856
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Explore data in Colab

Fundamental parameters

Reference Values
Cantat-Gaudin et al. (2020) AVNN=1.2, DistPc=876.0, AgeNN=7.29
He et al. (2022) A0=1.55, logAge=6.9
Celli et al. (2024) Age=19.5, Mc=141.6
Alfonso et al. (2024) AV=1.19907, MOD=9.70984, logAge=7.61589, Z=0.01004

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Riddle 6 100.0 318.03 59.9 1.17 -2.53 -3.51 -23.22 0.71
OC 0158 14.3 318.24 59.51 1.16 -2.54 -3.51 -24.65 0.03
CWNU 1192 5.7 318.54 59.41 1.16 -2.51 -3.5 -25.37 0.02