Loden 306

(MWSC 1889)

0.16 UTI

0.0

C_N

0.03

C_dens

0.25

C_C3

0.26

C_lit

1.0

C_dup

N_m (P>50%) 16

Core radius and density 3.3 [pc], 0.1 [pc^-2]

C3 classification DB

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.25 Low quality
C_lit 0.26 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Loden 306 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a massive, very young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~5.08 kpc) differs significantly from the median photometric distance (~1.97 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 Massive Very young

Data

🔍 Search references for Loden 306 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–	166.514	-61.141	0.197	-6.47	2.654	2.581
Just et al.	2023	166.479	-61.116	–	–	–	–
Dib et al.	2018	166.485	-61.12	–	–	–	–
Sampedro et al.	2017	166.533	-61.1	–	-2.52	-3.45	–
Kharchenko et al.	2016	166.479	-61.116	–	–	–	–
Dias et al.	2014	166.533	-61.1	–	-2.62	-3.39	–
Kharchenko et al.	2013	166.485	-61.12	–	-6.09	2.84	-33.0
Gozha et al.	2012	166.533	-61.1	–	–	–	–
Piskunov et al.	2008	166.495	-61.131	–	–	–	–
Kharchenko et al.	2007	166.53	-61.1	–	0.2	–	-33.0
Kharchenko et al.	2005	166.5	-61.13	–	-6.95	0.34	-33.0

💡 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–	1.97	1.085	–	6	–	1490	–	–
Just et al.	2023	–	–	–	6	–	635	–	–
Dib et al.	2018	1.94	–	–	6	–	–	–	–
Kharchenko et al.	2016	1.94	1.41	–	6	–	–	–	–
Kharchenko et al.	2013	1.94	1.41	–	6	–	–	–	–
Gozha et al.	2012	2.00	–	–	6	–	2344	–	–
Piskunov et al.	2008	2.00	0.76	–	6	–	–	–	–
Kharchenko et al.	2005	2.00	0.76	–	6	–	–	–	–

Visualization

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