Collinder 466

(MWSC 1102)

0.27 UTI

0.0

C_N

0.07

C_dens

0.38

C_C3

0.45

C_lit

1.0

C_dup

N₅₀ (P>50% members) 15

Stellar density (N₅₀/rad) 0.4 [N/pc²]

C3 classification BC

C_N 0.0 Sparse
C_dens 0.07 Very loose
C_C3 0.38 Low quality
C_lit 0.45 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Collinder 466 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by low 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 (~2.12 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 Low extinction Intermediate age

Data

🔍 Search references for Collinder 466 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–	106.746	-10.709	0.251	-1.033	0.452	88.719
Just et al.	2023	106.728	-10.718	–	–	–	–
Loktin & Popova	2017	106.74	-10.73	–	-0.717	0.011	–
Kharchenko et al.	2016	106.728	-10.718	–	–	–	–
Dias et al.	2014	106.733	-10.715	–	-0.1	0.82	–
Kharchenko et al.	2013	106.734	-10.72	–	0.64	1.23	–
Bukowiecki et al.	2011	106.733	-10.7	–	–	–	–
Dias et al.	2002	106.733	-10.715	–	-0.1	0.82	–

💡 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–	2.12	0.95	–	442	–	159	–	–
Just et al.	2023	–	–	–	254	–	6	–	–
Loktin & Popova	2017	2.69	0.95	–	851	–	–	–	–
Kharchenko et al.	2016	1.04	0.19	–	254	–	–	–	–
Kharchenko et al.	2013	1.04	0.19	–	254	–	–	–	–
Bukowiecki et al.	2012	–	–	–	–	–	312	–	–
Bukowiecki et al.	2011	2.55⁽¹⁾	1.40	–	631	–	–	–	–
Dias et al.	2002	2.12	1.43	–	631	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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