Loden 2326

(MWSC 2313)

0.23 UTI

0.0

C_N

0.01

C_dens

0.38

C_C3

0.38

C_lit

1.0

C_dup

C3 classification BC

Number of members (P>50%) 6

Radius (P>50% members) 7.5 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.38 Low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

ℹ️

Loden 2326 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.89 kpc) differs significantly from the median photometric distance (~1.15 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 Low mass Intermediate age

Data

🔍 Search references for Loden 2326 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	235.927	-52.446	0.17	-5.706	-4.524	-134.714
Just et al.	2023	235.901	-52.468	–	–	–	–
Bica et al.	2019	235.888	-52.469	–	–	–	–
Kharchenko et al.	2016	235.901	-52.468	–	–	–	–
Kharchenko et al.	2013	235.912	-52.47	–	-7.0	-3.33	–
van den Bergh	2006	235.887	-52.475	–	–	–	–
Dias et al.	2002	235.887	-52.475	–	-3.33	-6.48	–

💡 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	–	–	–	676	–	41	–	–
Kharchenko et al.	2016	1.39	1.78	–	676	–	–	–	–
Kharchenko et al.	2013	1.39	1.78	–	676	–	–	–	–
van den Bergh	2006	0.90	1.27	–	200	–	–	–	–
Dias et al.	2002	0.90	1.27	–	200	–	–	–	–

Visualization

ℹ️