LISC-III 1790

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C3
N_50
r_50
CC 13 8.7
Summary

LISC-III 1790 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It was recently reported in the literature.

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
Chi et al. (2023) 94.868 32.787 0.308 0.3 -1.78
           
UCC 94.868 32.705 0.232 0.215 -1.818 7.687
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

LISC-III 1790 UCC

Explore data in Colab

Fundamental parameters

Reference Values
Chi et al. (2023) E(V-I)=0.28, m-M=12.6, Z=0.02, fbin=0.5

Search coordinates in Bayestar19

Cluster region map