Dolidze 49

(MWSC 984)

0.18 UTI

0.0

C_N

0.29

C_dens

0.12

C_C3

0.25

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 19

Radius (P>50% members) 3.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.29 Loose
C_C3 0.12 Very low quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Dolidze 49 is a sparse, 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 an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~3.99 kpc) differs significantly from the median photometric distance (~2.40 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 Intermediate age

Data

🔍 Search references for Dolidze 49 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	–	101.742	-0.035	0.251	-0.931	1.214	–
Just et al.	2023	101.753	-0.009	–	–	–	–
Kharchenko et al.	2016	101.753	-0.009	–	–	–	–
Kharchenko et al.	2013	101.76	-0.01	–	-1.06	-2.17	–
Dias et al.	2002	101.767	-0.007	–	-1.06	-2.17	–

💡 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	–	–	–	214	–	283	–	–
Kharchenko et al.	2016	2.40	1.94	–	214	–	–	–	–
Kharchenko et al.	2013	2.40	1.94	–	214	–	–	–	–
Dias et al.	2002	2.40	1.94	–	214	–	–	–	–

Visualization

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