Dol Dzim 9

(DoDz 9; Dolidze-Dzimselejsvili 9; OCL 119; MWSC 2818)

Click to load Aladin Lite
0.05 UTI
0.0
CN
0.11
Cdens
0.12
CC3
0.0
Clit
1.0
Cdup
Stellar density (N50/rad) 0.6 [N/pc2]
  • CN 0.0 Sparse
  • Cdens 0.11 Very loose
  • CC3 0.12 Very low quality
  • Clit 0.0 Rarely studied
  • Cdup 1.0 Unique

Overview

â„šī¸
Dol Dzim 9 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 7 years.

(*): The parallax distance estimate (~3.48 kpc) differs significantly from the median photometric distance (~2.33 kpc).

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

â„šī¸
Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 272.201 31.577 0.288 -2.235 -3.633 –
Bica et al. 2019 272.121 31.587 – – – –
Dias et al. 2014 272.2 31.533 – -0.28 -1.19 –
Dias et al. 2002 272.2 31.533 – -0.28 -1.19 –

💡 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– 2.33 0.19 – 2291 – – – –
Dias et al. 2002 2.33 0.19 – 2291 – – – –

Visualization

â„šī¸