UBC 392

Click to load Aladin Lite
C3
N_50
r_50
CA 48 8.2
Summary

UBC 392 is a poorly populated, very dense object of intermediate 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) 336.117 64.931 1.056 -0.643 -3.275
Cantat-Gaudin et al. (2020) 336.125 64.926 1.056 -0.642 -3.287
He et al. (2022) 336.726 65.067 1.068 -1.091 -2.889
Alfonso et al. (2024) 336.481 65.01 1.039 -0.89 -2.988
           
UCC 336.129 64.944 1.06 -0.646 -3.342 -8.82
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=1.47, DistPc=965.0, AgeNN=7.85
Tarricq et al. (2022) Dist=941, logAgeNN=7.93
He et al. (2022) A0=2.45, logAge=7.1
Alfonso et al. (2024) AV=1.47005, MOD=9.91942, logAge=7.49966, Z=0.01067

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UPK 194 100.0 336.32 64.98 1.06 -0.63 -3.28 -11.95 0.8