Dolidze 38

(MWSC 3251)

0.36 UTI

0.39

C_N

0.03

C_dens

0.38

C_C3

0.5

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 39

Radius (P>50% members) 6.5 [arcmin]

C_N 0.39 Poorly populated
C_dens 0.03 Very loose
C_C3 0.38 Low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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Dolidze 38 is a poorly populated, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well above the mid-plane, affected by low extinction. It is catalogued as an old cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~7.91 kpc) differs significantly from the median photometric distance (~1.36 kpc).

Relatively close Low extinction Old

Data

🔍 Search references for Dolidze 38 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	–	301.484	41.177	0.126	-3.016	-3.466	-28.186
Just et al.	2023	301.465	41.193	–	–	–	–
Loktin & Popova	2017	301.425	41.2	–	-0.675	-0.348	–
Kharchenko et al.	2016	301.465	41.193	–	–	–	–
Dias et al.	2014	301.425	41.2	–	-1.73	-6.11	–
Kharchenko et al.	2013	301.47	41.195	–	-2.82	-1.41	–
Piskunov et al.	2008	301.389	41.196	–	–	–	–
Kharchenko et al.	2005	301.39	41.2	–	-3.59	-6.49	–
Dias et al.	2002	301.425	41.2	–	-1.73	-6.11	–

💡 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	–	–	–	1462	–	403	–	–
Loktin & Popova	2017	3.29	0.72	–	2239	–	–	–	–
Kharchenko et al.	2016	1.53	0.71	–	1462	–	–	–	–
Kharchenko et al.	2013	1.53	0.71	–	1462	–	–	–	–
Piskunov et al.	2008	1.20	0.46	–	891	–	–	–	–
Kharchenko et al.	2005	1.20	0.46	–	891	–	–	–	–
Dias et al.	2002	1.20	0.46	–	891	–	–	–	–

Visualization

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