UBC 17 b

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C3
N_50
r_50
AA 179 16.8
Summary

UBC 17 b is a rich, very dense object of very high C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It is poorly studied in the literature.

This object shares a large percentage of members with 3 later reported entries.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Castro-Ginard et al. (2018) 83.355 -1.548 2.363 0.055 -0.167 33.19
Cantat-Gaudin et al. (2020) 83.195 -1.585 2.376 0.078 -0.163
Celli et al. (2024) 83.195 -1.585
Alfonso et al. (2024) 83.2 -1.72 2.36 0.045 -0.209
           
UCC 83.165 -1.709 2.396 0.07 -0.218 25.619
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=0.05, DistPc=408.0, AgeNN=7.06
Celli et al. (2024) Age=11.5, Mc=173.7
Alfonso et al. (2024) AV=0.05287, MOD=7.94787, logAge=6.98030, Z=-0.0348

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Gulliver 6 100.0 83.34 -1.63 2.41 -0.07 -0.24 28.06 0.68
OCSN 194 100.0 83.32 -1.64 2.42 -0.06 -0.25 28.06 0.02
Theia 13 54.7 83.14 -1.76 2.4 0.08 -0.22 25.77 0.0