Loden 1373

(MWSC 2243; OCL 923.1)

0.20 UTI

0.0

C_N

0.02

C_dens

0.38

C_C3

0.31

C_lit

1.0

C_dup

C3 classification CB

Number of members (P>50%) 11

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.02 Very loose
C_C3 0.38 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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Loden 1373 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.45 kpc) differs significantly from the median photometric distance (~3.41 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 High extinction Massive Young

Data

🔍 Search references for Loden 1373 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	–	220.343	-62.854	0.225	-6.832	-4.034	-46.003
Just et al.	2023	220.381	-62.888	–	–	–	–
Bica et al.	2019	220.433	-62.848	–	–	–	–
Kharchenko et al.	2016	220.381	-62.888	–	–	–	–
Dias et al.	2014	220.45	-62.867	–	-8.51	0.01	–
Kharchenko et al.	2013	220.395	-62.89	–	-5.57	0.1	–

💡 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	–	–	–	89	–	3155	–	–
Kharchenko et al.	2016	3.41	3.23	–	89	–	–	–	–
Kharchenko et al.	2013	3.41	3.23	–	89	–	–	–	–

Visualization

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