GLIMPSE 70

(Mercer 70; Ryu 273)

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.5 0.26 0.38 0.0 0.9
C3
N_50
r_50
BC 50 7.8
Summary

GLIMPSE 70 is a moderately populated, loose object of low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.

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

Warning: the low UTI value and no obvious signs of duplication (C_dup=0.9) 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
Bica et al. (2019) 240.123 -52.182 – – – –
           
UCC 240.139 -52.163 0.369 -5.002 -4.118 -23.134
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

GLIMPSE 70 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
MCM 70 10.0 240.12 -52.18 0.31 -4.34 -4.26 -42.09 0.32