Dolidze 14

(OCL 425; MWSC 330)

0.22 UTI

0.27

C_N

0.01

C_dens

0.5

C_C3

0.16

C_lit

1.0

C_dup

N_m (P>50%) 27

Core radius and density 10 [pc], 0.03 [pc^-2]

C3 classification BB

C_N 0.27 Poorly populated
C_dens 0.01 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.16 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Dolidze 14 is a poorly populated, very loose object of intermediate C3 quality. Its parallax locates it at a very large^* distance, well below 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 (~10.43 kpc) differs significantly from the median photometric distance (~1.70 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 Low extinction Old

Data

🔍 Search references for Dolidze 14 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–	61.629	27.51	0.096	0.754	-0.92	-13.723
Bica et al.	2019	61.651	27.529	–	–	–	–
Dias et al.	2018	–	–	–	1.41	-4.37	–
Loktin & Popova	2017	61.68	27.543	–	0.151	-6.232	–
Sampedro et al.	2017	61.679	27.543	–	2.28	-0.54	–
Dias et al.	2014	61.679	27.543	–	1.71	-0.88	–
Dias et al.	2002	61.679	27.543	–	1.71	-0.88	–
Lynga	1987	61.641	27.439	–	–	–	–

💡 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–	1.695	0.835	–	1153	–	–	–	–
Loktin & Popova	2017	1.72	0.66	–	1047	–	–	–	–
Dias et al.	2002	1.67	1.01	–	1259	–	–	–	–

Visualization

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