Dolidze 37

(MWSC 3235)

0.17 UTI

0.0

C_N

0.0

C_dens

0.12

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 12

Stellar density (N₅₀/rad) 0.0 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.0 Very loose
C_C3 0.12 Very low quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Dolidze 37 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by very high extinction. It is catalogued as a young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.29 kpc) differs significantly from the median photometric distance (~1.40 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 Very high extinction Young

Data

🔍 Search references for Dolidze 37 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–	300.705	37.65	0.137	-3.748	-5.938	-34.165
Just et al.	2023	300.708	37.647	–	–	–	–
Loktin & Popova	2017	300.72	37.654	–	-3.608	-7.549	–
Kharchenko et al.	2016	300.708	37.647	–	–	–	–
Dias et al.	2014	300.75	37.683	–	-0.16	-3.42	–
Kharchenko et al.	2013	300.712	37.65	–	-3.66	-3.61	–
Dias et al.	2002	300.75	37.683	–	-0.16	-3.42	–

💡 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–	1.4	7.16	–	38	–	149	–	–
Just et al.	2023	–	–	–	38	–	149	–	–
Loktin & Popova	2017	1.92	0.92	–	708	–	–	–	–
Kharchenko et al.	2016	1.40	7.16	–	38	–	–	–	–
Kharchenko et al.	2013	1.40	7.16	–	38	–	–	–	–
Dias et al.	2002	1.40	7.16	–	38	–	–	–	–

Visualization

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