Dolidze 44

0.12 UTI

0.0

C_N

0.02

C_dens

0.25

C_C3

0.16

C_lit

1.0

C_dup

N_m (P>50%) 18

Core radius and density 1.6 [pc], 0.1 [pc^-2]

C3 classification CC

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.25 Low 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 44 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

⚠️ 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 44 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–	307.371	41.7	0.523	-3.108	-4.661	29.862
Dias et al.	2018	–	–	–	-1.32	-3.15	–
Dib et al.	2018	307.447	41.635	–	–	–	–
Loktin & Popova	2017	307.425	41.717	–	0.165	-0.773	–
Sampedro et al.	2017	307.425	41.717	–	-0.71	-5.54	–
Joshi et al.	2016	307.447	41.635	–	–	–	–
Dias et al.	2002	307.425	41.717	–	-0.61	-5.44	–
Lynga	1987	307.411	41.717	–	–	–	–

💡 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–	1.5	2.17	–	143	–	–	–	–
Dib et al.	2018	1.50	–	–	143	–	–	–	–
Loktin & Popova	2017	1.10	1.31	–	234	–	–	–	–
Joshi et al.	2016	1.50	2.17	–	143	–	–	–	–
Dias et al.	2002	1.50	2.17	–	143	–	–	–	–

Visualization

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