Loden 153

(MWSC 1824)

0.24 UTI

0.0

C_N

0.06

C_dens

0.12

C_C3

0.5

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 16

Radius (P>50% members) 7.4 [arcmin]

C_N 0.0 Sparse
C_dens 0.06 Very loose
C_C3 0.12 Very low quality
C_lit 0.5 Moderately studied
C_dup 1.0 Unique

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

Overview

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Loden 153 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 a near-solar metallicity, very young cluster (see Parameters). It is moderately studied in the literature.

⚠️ 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 Near-solar metallicity Very young

Data

🔍 Search references for Loden 153 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	–	158.657	-58.14	0.306	-6.019	2.41	31.432
Just et al.	2023	158.664	-58.126	–	–	–	–
Kharchenko et al.	2016	158.664	-58.126	–	–	–	–
Dias et al.	2014	158.675	-58.133	–	-4.95	0.06	–
Kharchenko et al.	2013	158.67	-58.13	–	-7.11	4.36	-10.3
Gozha et al.	2012	158.675	-58.133	–	–	–	–
Piskunov et al.	2008	158.672	-58.123	–	–	–	–
Kharchenko et al.	2007	158.67	-58.13	–	0.1	–	-10.33
Kharchenko et al.	2005	158.67	-58.13	–	-5.85	4.13	-10.33

💡 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	–	–	–	2	–	239	–	–
Kharchenko et al.	2016	3.02	1.00	–	2	–	–	–	–
Kharchenko et al.	2013	3.02	1.00	–	2	0.191	–	–	–
Gozha et al.	2012	2.67	–	–	5	–	1514	–	–
Piskunov et al.	2008	2.67	0.87	–	5	–	–	–	–
Kharchenko et al.	2005	2.67	0.87	–	5	–	–	–	–

Visualization

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