Dolidze 10

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0.19 UTI
0.0
CN
0.59
Cdens
0.38
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 3.0 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.59 Moderately dense
  • CC3 0.38 Low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

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Dolidze 10 is a sparse, moderately dense object of low C3 quality. Its parallax locates it at a relatively close* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 12 years.

(*): The parallax distance estimate (~1.94 kpc) differs significantly from the median photometric distance (~950.00 kpc).

Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.

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– 306.589 40.184 0.515 -2.115 -3.159 -43.538
Tadross 2014 306.575 40.117 – – – –

💡 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– 950.0 2.48 – 250 – – – –
Tadross 2014 950.00 2.48 – 250 – – – –
Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWNU 4207 16.0 306.56 40.26 0.36 -2.23 -3.86 -20.55 0.0
HSC 619 16.0 306.56 40.25 0.36 -2.23 -3.86 -20.55 0.4

💡 Note: The % column shows the percentage of members that Dolidze 10 shares with each listed object.

Visualization

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