Dolidze 21

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0.15 UTI
0.0
CN
0.02
Cdens
0.25
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 0.1 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.02 Very loose
  • CC3 0.25 Low quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Dolidze 21 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large distance, well below the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature, with no articles listed in the last 12 years.

âš ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 81.896 7.081 0.199 0.709 -0.432 34.469
Dias et al. 2014 81.85 7.067 – 0.17 0.53 –
Bukowiecki et al. 2011 81.912 7.117 – – – –
Dias et al. 2002 81.85 7.067 – 0.17 0.53 –

💡 Note: The UCC values are estimated from its identified members.

Reference Year Dist [kpc] Av [mag] DAv [mag] Age [Myr] [Fe/H] [dex] Mass [Msun] Bfrac BSS
UCC 99999– 4.745 3.815 – 178 – 183 – –
Bukowiecki et al. 2012 – – – – – 183 – –
Bukowiecki et al. 2011 5.89(1) 3.75 – 178 – – – –
Dias et al. 2002 3.60 3.88 – 178 – – – –

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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