NGC 6828

(MWSC 3190)

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C3
N_50
r_50
DC 15 8.2
Summary

NGC 6828 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is moderately studied in the literature.

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

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Positions

Reference RA DEC Plx pmRA pmDE Rv
Kharchenko et al. (2005) 297.57 7.9 -1.12 -2.9 -21.0
Kharchenko et al. (2007) 297.57 7.9 0.18 -21.0
Piskunov et al. (2008) 297.561 7.896
Kharchenko et al. (2013) 297.562 7.905 0.05 -4.35 -21.0
Kharchenko et al. (2016) 297.556 7.903
Loktin & Popova (2017) 297.54 7.905 -2.123 -4.756 -21.0
Bica et al. (2019) 297.561 7.896
Just et al. (2023) 297.556 7.903
           
UCC 297.555 7.95 0.251 -1.798 -2.908 -54.178
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

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Estimated members

NGC 6828 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2005) E(B-V)=0.2, Dist=600, logt=8.56
Piskunov et al. (2008) E(B-V)=0.2, Dist=600, logt=8.56, logMA=1.424
Kharchenko et al. (2013) E(B-V)=0.167, d=603.0, logt=8.25
Kharchenko et al. (2016) E(B-V)=0.167, d=603.0, logt=8.25
Loktin & Popova (2017) E(B-V)=0.215, Dist=2803, logt=9.34
Just et al. (2023) logt=8.25, logmt=1.169

Search coordinates in Bayestar19

Cluster region map