FSR 1766

(MWSC 2630)

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C3
N_50
r_50
BB 13 5.0
Summary

FSR 1766 is a sparse, very loose object of intermediate C3 quality. It is located at a very large distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.

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
Froebrich et al. (2007) 263.625 -36.65
Kharchenko et al. (2012) 263.64 -36.65 -4.22 -1.13
Bica et al. (2019) 263.625 -36.653
           
UCC 263.656 -36.707 0.08 -2.579 -5.106 -119.095
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

FSR 1766 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=1.103, distance=3540, log_age=9.125

Search coordinates in Bayestar19

Cluster region map