Loden 480

(MWSC 1986; OCL 865.3)

0.50 UTI

0.41

C_N

0.29

C_dens

0.62

C_C3

0.6

C_lit

1.0

C_dup

C3 classification AC

Number of members (P>50%) 41

Radius (P>50% members) 24.7 [arcmin]

C_N 0.41 Poorly populated
C_dens 0.29 Loose
C_C3 0.62 Intermediate quality
C_lit 0.6 Moderately studied
C_dup 1.0 Unique

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

Overview

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Loden 480 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a close^* distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~0.74 kpc) differs significantly from the median photometric distance (~1.20 kpc).

Relatively close Low extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as a moving group.

Data

🔍 Search references for Loden 480 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	–	179.266	-58.324	1.342	-9.835	-0.707	-5.539
Cavallo et al.	2024	179.686	-58.345	1.369	–	–	–
Hunt & Reffert	2023	179.317	-58.3	1.363	-9.848	-0.687	-7.488
Just et al.	2023	178.896	-58.387	–	–	–	–
Bica et al.	2019	179.165	-58.349	–	–	–	–
Kharchenko et al.	2016	178.896	-58.387	–	–	–	–
Dias et al.	2014	179.0	-58.433	–	-7.78	2.47	–
Kharchenko et al.	2013	178.905	-58.39	–	-9.03	4.4	–
Piskunov et al.	2008	178.988	-58.401	–	–	–	–
Kharchenko et al.	2005	178.99	-58.4	–	-10.56	2.94	–
Kharchenko et al.	2003	178.99	-58.4	–	-8.55	5.73	–

💡 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
Cavallo et al.	2024	0.73	0.67	–	347	-0.010	–	–	–
Hunt & Reffert	2023	0.69	0.27	0.49	220	–	–	–	–
Just et al.	2023	–	–	–	501	–	54	–	–
Kharchenko et al.	2016	1.30	0.64	–	501	–	–	–	–
Kharchenko et al.	2013	1.30	0.64	–	501	–	–	–	–
Piskunov et al.	2008	1.20	0.93	–	513	–	–	–	–
Kharchenko et al.	2005	1.20	0.93	–	513	–	–	–	–
Kharchenko et al.	2003	1.43	1.24	–	–	–	–	–	–

Visualization

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