MWSC 4409

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C3
N_50
r_50
BC 25 7.3
Summary

MWSC 4409 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.

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
Kharchenko et al. (2012) 273.84 31.725 0.29 -4.72
Bica et al. (2019) 273.834 31.725
           
UCC 273.855 31.725 0.214 -2.317 -3.422 -114.591
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

MWSC 4409 UCC

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Fundamental parameters

Reference Values
Kharchenko et al. (2012) e_bv=0.656, distance=2740, log_age=8.85

Search coordinates in Bayestar19

Cluster region map