Dolidze 56

(MWSC 3583)

0.13 UTI

0.0

C_N

0.02

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 7

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Dolidze 56 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

⚠️ 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.

Very distant High extinction Intermediate age

Dias et al. (2002)
Asterism (Kronberger, M. 2007, private communication); cat V3.5 (Jan 2016)

Data

🔍 Search references for Dolidze 56 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–	331.134	59.889	0.195	-2.44	-2.019	-55.855
Just et al.	2023	331.022	59.896	–	–	–	–
Kharchenko et al.	2016	331.022	59.896	–	–	–	–
Kharchenko et al.	2013	331.027	59.9	–	-2.78	-1.0	–
Kharchenko et al.	2012	331.027	59.9	–	-2.78	-1.0	–

💡 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–	7.0	3.1	–	891	–	294	–	–
Just et al.	2023	–	–	–	891	–	294	–	–
Kharchenko et al.	2016	7.00	3.10	–	891	–	–	–	–
Kharchenko et al.	2013	7.00	3.10	–	891	–	–	–	–
Kharchenko et al.	2012	7.00	3.10	–	891	–	–	–	–

Visualization

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