Dolidze 37

(MWSC 3235)

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C3
N_50
r_50
DC 12 10.4
Summary

Dolidze 37 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, above 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) 300.75 37.683 -0.16 -3.42
Kharchenko et al. (2013) 300.712 37.65 -3.66 -3.61
Kharchenko et al. (2016) 300.708 37.647
Loktin & Popova (2017) 300.72 37.654 -3.608 -7.549
Just et al. (2023) 300.708 37.647
           
UCC 300.705 37.65 0.137 -3.748 -5.938 -34.165
Galactocentric position Galactocentric position diagram

How are the galactocentric plots generated?

Search coordinates in CDS | Simbad

Estimated members

Dolidze 37 UCC

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Fundamental parameters

Reference Values
Dias et al. (2002) E(B-V)=2.311, Dist=1400.0, Age=7.585
Kharchenko et al. (2013) E(B-V)=2.311, d=1400.0, logt=7.585
Kharchenko et al. (2016) E(B-V)=2.311, d=1400.0, logt=7.585
Loktin & Popova (2017) E(B-V)=0.297, Dist=1919, logt=8.85
Just et al. (2023) logt=7.585, logmt=2.172

Search coordinates in Bayestar19

Cluster region map