Dol Dzim 11

(MWSC 3415; DoDz 11; Dolidze-Dzimselejsvili 11; OCL 179)

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C3
N_50
r_50
DC 13 7.7
Summary

Dol Dzim 11 is a sparse, very loose object of very 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.

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) 312.75 35.95 -2.22 -2.6
Kharchenko et al. (2013) 312.778 35.945 -0.97 -2.14
Kharchenko et al. (2016) 312.773 35.942
Bica et al. (2019) 312.759 35.881
Just et al. (2023) 312.773 35.942
           
UCC 312.731 35.918 0.135 -3.123 -3.855 -111.541
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Dol Dzim 11 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=0.42, Dist=2545.0, Age=9.3
Kharchenko et al. (2013) E(B-V)=0.5, d=4873.0, logt=9.2
Kharchenko et al. (2016) E(B-V)=0.5, d=4873.0, logt=9.2
Just et al. (2023) logt=9.2, logmt=2.678

Search coordinates in Bayestar19

Cluster region map