Loden 165

0.08 UTI

0.0

C_N

0.06

C_dens

0.0

C_C3

0.16

C_lit

1.0

C_dup

N₅₀ (P>50% members) 18

Stellar density (N₅₀/rad) 0.3 [N/pc²]

C3 classification DD

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.0 Very low quality
C_lit 0.16 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Loden 165 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~3.29 kpc) differs significantly from the median photometric distance (~1.33 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 Loden 165 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–	158.986	-58.749	0.304	-5.932	-2.247	13.941
Dias et al.	2018	–	–	–	-6.94	2.13	–
Dib et al.	2018	158.983	-58.733	–	–	–	–
Sampedro et al.	2017	158.983	-58.737	-5.59	-3.16	–	–
Joshi et al.	2016	158.983	-58.733	–	–	–	–
Dias et al.	2014	158.983	-58.737	–	-5.81	-3.14	–
Dias et al.	2002	158.983	-58.737	–	-5.81	-3.14	–
Lynga	1987	158.672	-58.643	–	–	–	–

💡 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–	1.33	0.79	–	178	–	–	–	–
Dib et al.	2018	1.33	–	–	178	–	–	–	–
Joshi et al.	2016	1.33	0.79	–	178	–	–	–	–
Dias et al.	2002	1.90	0.79	–	3020	–	–	–	–

Visualization

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