Dol Dzim 2

(MWSC 525)

0.18 UTI

0.0

C_N

0.05

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 15

Radius (P>50% members) 6.1 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 Very loose
C_C3 0.25 Low quality
C_lit 0.31 Poorly studied
C_dup 1.0 Unique

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

Overview

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Dol Dzim 2 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.38 kpc) differs significantly from the median photometric distance (~1.37 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

Data

🔍 Search references for Dol Dzim 2 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	–	80.955	11.512	0.228	0.235	-0.731	12.845
Just et al.	2023	80.962	11.491	–	–	–	–
Kharchenko et al.	2016	80.962	11.491	–	–	–	–
Dias et al.	2014	80.975	11.467	–	4.04	-3.5	–
Kharchenko et al.	2013	80.97	11.49	–	1.96	-8.01	–
Dias et al.	2002	80.975	11.467	–	4.04	-3.5	–

💡 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	–	–	–	1059	–	113	–	–
Kharchenko et al.	2016	1.37	2.06	–	1059	–	–	–	–
Kharchenko et al.	2013	1.37	2.06	–	1059	–	–	–	–
Dias et al.	2002	1.22	2.02	–	794	–	–	–	–

Visualization

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