G 80.35+0.72

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C3
N_50
r_50
CB 24 3.4
Summary

G 80.35+0.72 is a sparse, very dense object of low C3 quality. It is located at a relatively close distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.

This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry.

Warning: contains less than 25 stars with P>0.5 estimated.

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.6) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2012) 308.475 41.382 -1.1 -0.07
           
UCC 308.432 41.377 0.545 -2.825 -4.128 -4.792
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

G 80.35+0.72 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=0.822, distance=1089, log_age=7.5

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
Cyg OB2 40.0 308.31 41.3 0.58 -2.72 -4.41 -8.19 0.14
FSR 0238 24.0 308.63 41.39 0.59 -2.84 -4.53 -27.33 0.87
Bica 2 20.0 308.31 41.3 0.58 -2.68 -4.41 -13.56 0.79
FSR 0236 4.0 308.15 41.43 0.57 -2.41 -4.11 55.7 0.66