Mayer 2

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UTI:
UCC Trust Index

C_N C_dens C_C3 C_lit C_dup
0.0 0.04 0.25 0.0 1.0
C3
N_50
r_50
CC 16 8.3
Summary

Mayer 2 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 8 years.

This object shares a small 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
Dias et al. (2002) 64.938 53.167 – -1.41 -5.88 –
Loktin & Popova (2017) 64.935 53.168 – -2.923 1.264 –
           
UCC 64.996 53.161 0.255 0.312 -0.719 -25.204
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Mayer 2 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.06, Dist=1589.0, Age=7.4
Loktin & Popova (2017) E(B-V)=0.882, Dist=3062, logt=7.51

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

Cluster % RA DEC Plx pmRA pmDE Rv UTI
UBC 609 16.0 65.23 53.05 0.22 0.46 -0.73 – 0.22