Dol Dzim 6

(Dolidze-Dzimselejsvili 6)

0.10 UTI

0.25

C_N

0.01

C_dens

0.12

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 25

Core radius and density 5.6 [pc], 0.04 [pc^-2]

C3 classification DC

C_N 0.25 Poorly populated
C_dens 0.01 Very loose
C_C3 0.12 Very low quality
C_lit 0.06 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

MOCA 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Dol Dzim 6 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by low extinction. It is catalogued as a very old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 10 years.

(*): The parallax distance estimate (~7.58 kpc) differs significantly from the median photometric distance (~0.82 kpc).

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

Close Low extinction Very old

Data

🔍 Search references for Dol Dzim 6 in: SciX Simbad

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Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	251.413	38.352	0.132	-1.887	-2.368	–
Joshi et al.	2016	251.377	38.36	–	–	–	–
Tadross	2014	251.35	38.35	–	–	–	–
Dias et al.	2002	251.35	38.35	–	9.51	2.86	-46.1
Lynga	1987	251.327	38.28	–	–	–	–

💡 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]	B_frac	BSS
UCC	99999–	0.82	0.09	–	5000	–	–	–	–
Joshi et al.	2016	0.95	0.20	–	2818	–	–	–	–
Tadross	2014	0.82	0.09	–	5000	–	–	–	–
Dias et al.	2002	0.82	0.09	–	5012	–	–	–	–

Visualization

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