Dolidze 45

0.13 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.13

C_lit

1.0

C_dup

N_m (P>50%) 17

Core radius and density 7.5 [pc], 0.04 [pc^-2]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.38 Low quality
C_lit 0.13 Rarely studied
C_dup 1.0 Unique

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

Overview

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Dolidze 45 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~7.36 kpc) differs significantly from the median photometric distance (~2.46 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 Old

Bica et al. (2019)
Analysis of Dolidze objects by M. Kronberger reported in DAML02. Asterisms reported by amateur astronomers in the web.

Data

🔍 Search references for Dolidze 45 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–	317.707	37.565	0.136	-2.213	-3.619	–
Dias et al.	2018	–	–	–	-3.06	-4.71	–
Loktin & Popova	2017	317.7	37.534	–	-0.684	-0.667	–
Sampedro et al.	2017	317.692	37.574	–	-0.15	-3.31	–
Dias et al.	2014	317.692	37.574	–	-0.12	-3.08	–
Dias et al.	2002	317.692	37.574	–	-0.12	-3.08	–
Lynga	1987	317.244	37.603	–	–	–	–

💡 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–	2.46	1.02	–	1524	–	–	–	–
Loktin & Popova	2017	1.99	0.40	–	2188	–	–	–	–
Dias et al.	2002	2.93	1.64	–	861	–	–	–	–

Visualization

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