Dolidze 52

(MWSC 2907)

0.21 UTI

0.0

C_N

0.19

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 14

Radius (P>50% members) 6.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.19 Very loose
C_C3 0.12 Very 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 52 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.12 kpc) differs significantly from the median photometric distance (~1.32 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 Young

Data

🔍 Search references for Dolidze 52 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	–	276.057	-16.699	0.471	-1.94	-2.704	4.074
Just et al.	2023	275.973	-16.642	–	–	–	–
Loktin & Popova	2017	275.985	-16.64	–	1.297	-5.319	–
Kharchenko et al.	2016	275.973	-16.642	–	–	–	–
Dias et al.	2014	275.975	-16.65	–	0.75	-4.21	–
Kharchenko et al.	2013	275.98	-16.64	–	1.26	-6.54	–
Dias et al.	2002	275.975	-16.65	–	0.75	-4.21	–

💡 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	–	–	–	20	–	71	–	–
Loktin & Popova	2017	2.08	1.56	–	20	–	–	–	–
Kharchenko et al.	2016	1.32	1.94	–	20	–	–	–	–
Kharchenko et al.	2013	1.32	1.94	–	20	–	–	–	–
Dias et al.	2002	1.32	1.94	–	20	–	–	–	–

Visualization

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