MCM 17

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.01 0.38 0.0 1.0
C3
N_50
r_50
BC 14 5.7
Summary

MCM 17 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, near the mid-plane. It is rarely studied in the literature, with no articles listed in the last 20 years.

This object shares a significant percentage of members with a later 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=1.0) 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
Mercer et al. (2005) 287.329 8.196 – – – –
UCC 287.315 8.17 0.113 -2.146 -4.522 50.857
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

MCM 17 UCC

Explore data in Colab

Search coordinates in Bayestar19

Cluster region


Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
GLIMPSE 17 60.0 287.27 8.12 0.12 -2.14 -4.54 40.51 0.03