ASCC 122

(MWSC 3637)

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C3
N_50
r_50
CC 23 6.4
Summary

ASCC 122 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, well 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
Dias et al. (2002) 338.308 39.61 -0.77 -5.05 -6.51
Piskunov et al. (2008) 338.306 39.611
Bica et al. (2019) 338.306 39.611
           
UCC 338.321 39.62 0.187 -2.951 -3.136
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

ASCC 122 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.1, Dist=700.0, Age=6.98
Piskunov et al. (2008) E(B-V)=0.1, Dist=700, logt=6.98, logMA=3.453

Search coordinates in Bayestar19

Cluster region map