NGC 6618

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C3
N_50
r_50
CC 20 28.1
Summary

NGC 6618 is a sparse, very loose object of low C3 quality. It is located at a close distance from the Sun, near the mid-plane. It is moderately studied in the literature.

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

Search object in SciX | Simbad

Positions

Reference RA DEC Plx pmRA pmDE Rv
Dias et al. (2002) 275.196 -16.172 1.51 -1.74 -25.3
Piskunov et al. (2007) 275.132 -16.19
Piskunov et al. (2008) 275.132 -16.19
Loktin & Popova (2017) 275.19 -16.173 1.51 -1.74 -4.0
Hunt & Reffert (2023) 275.065 -15.982 1.635 1.757 -5.381 -16.956
Cavallo et al. (2024) 275.479 -14.741 1.634
           
UCC 275.097 -15.456 1.626 1.81 -5.377 -16.67
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=1.51, Dist=1300.0, Age=6.0, [Fe/H]=0.132
Piskunov et al. (2007) E(B-V)=1.6, Dist=1814, logt=6.78, logM=2.923
Piskunov et al. (2008) E(B-V)=1.6, Dist=1814, logt=6.78, logM=4.026, logMA=4.479
Loktin & Popova (2017) E(B-V)=1.604, Dist=1814, logt=7.044
Hunt & Reffert (2023) AV50=1.126, diffAV50=1.465, MOD50=8.847, logAge50=8.591
Cavallo et al. (2024) AV50=1.53, dMod50=8.84, logAge50=8.32, [Fe/H]50=-0.05

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Cluster region map