ESO 367 10

(MWSC 1161)

0.18 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 17

Radius (P>50% members) 5.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.03 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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ESO 367 10 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well below 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 (~6.09 kpc) differs significantly from the median photometric distance (~3.03 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.

Distant Moderate extinction Intermediate age

Data

🔍 Search references for ESO 367 10 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	–	109.288	-35.329	0.164	-0.84	2.167	125.337
Just et al.	2023	109.255	-35.288	–	–	–	–
Loktin & Popova	2017	109.32	-35.32	–	-7.344	0.747	–
Kharchenko et al.	2016	109.255	-35.288	–	–	–	–
Kharchenko et al.	2013	109.26	-35.29	–	-5.06	-4.02	–
Dias et al.	2002	109.271	-35.28	–	-5.78	26.59	–

💡 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	–	–	–	207	–	69	–	–
Loktin & Popova	2017	2.75	1.00	–	851	–	–	–	–
Kharchenko et al.	2016	3.03	2.84	–	207	–	–	–	–
Kharchenko et al.	2013	3.03	2.84	–	207	–	–	–	–
Dias et al.	2002	3.03	2.84	–	207	–	–	–	–

Visualization

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