Dolidze 22

(FSR 1006; MWSC 854)

0.22 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.4

C_lit

1.0

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.4 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 22 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, below 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 (~7.06 kpc) differs significantly from the median photometric distance (~1.96 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for Dolidze 22 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–	95.859	4.59	0.142	0.109	-0.439	67.155
Just et al.	2023	95.802	4.592	–	–	–	–
Loktin & Popova	2017	95.835	4.6	–	-0.35	-0.69	–
Kharchenko et al.	2016	95.802	4.592	–	–	–	–
Dias et al.	2014	95.837	4.599	–	-0.35	-0.69	–
Kharchenko et al.	2013	95.809	4.59	–	-1.14	-1.42	–
Froebrich et al.	2007	95.737	4.626	–	–	–	–
Dias et al.	2002	95.838	4.599	–	-0.35	-0.69	–

💡 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–	1.96	1.48	–	234	–	112	–	–
Just et al.	2023	–	–	–	234	–	112	–	–
Loktin & Popova	2017	2.30	0.91	–	1023	–	–	–	–
Kharchenko et al.	2016	1.77	1.48	–	234	–	–	–	–
Kharchenko et al.	2013	1.77	1.48	–	234	–	–	–	–
Dias et al.	2002	2.15	2.08	–	355	–	–	–	–

Visualization

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