Dolidze 26

(MWSC 1246; OCL 516)

0.20 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.38

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 21

Radius (P>50% members) 7.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Dolidze 26 is a sparse, very loose object of low C3 quality. Its parallax locates it at a very large^* distance, well above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~11.60 kpc) differs significantly from the median photometric distance (~2.07 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.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for Dolidze 26 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	–	112.525	11.841	0.086	-0.219	-0.903	56.388
Just et al.	2023	112.512	11.888	–	–	–	–
Bica et al.	2019	112.516	11.894	–	–	–	–
Loktin & Popova	2017	112.515	11.886	–	-2.805	-2.346	–
Kharchenko et al.	2016	112.512	11.888	–	–	–	–
Dias et al.	2014	112.525	11.9	–	-0.02	-0.62	–
Kharchenko et al.	2013	112.519	11.885	–	-0.96	-2.99	–

💡 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]	Bfr	BSS
Just et al.	2023	–	–	–	299	–	395	–	–
Loktin & Popova	2017	3.99	0.13	–	1000	–	–	–	–
Kharchenko et al.	2016	2.07	1.16	–	299	–	–	–	–
Kharchenko et al.	2013	2.07	1.16	–	299	–	–	–	–

Visualization

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