Loden 807

(MWSC 2117)

0.42 UTI

0.3

C_N

0.34

C_dens

0.25

C_C3

0.6

C_lit

1.0

C_dup

N₅₀ (P>50% members) 30

Stellar density (N₅₀/rad) 1.7 [N/pc²]

C3 classification CC

C_N 0.3 Poorly populated
C_dens 0.34 Loose
C_C3 0.25 Low quality
C_lit 0.6 Moderately studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Loden 807 is a poorly populated, loose object of 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, intermediate-age cluster (see Parameters). It is moderately studied in the literature.

(*): The parallax distance estimate (~3.22 kpc) differs significantly from the median photometric distance (~0.93 kpc).

Close Low extinction Near-solar metallicity Intermediate age

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: one or a few submm emission within the cluster area.

Data

🔍 Search references for Loden 807 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–	201.149	-62.519	0.31	-8.001	-2.089	5.746
Just et al.	2023	201.147	-62.492	–	–	–	–
Loktin & Popova	2017	201.165	-62.483	–	-9.648	1.596	-0.1
Kharchenko et al.	2016	201.147	-62.492	–	–	–	–
Dias et al.	2014	201.167	-62.483	–	-7.55	-3.61	–
Kharchenko et al.	2013	201.157	-62.495	–	-6.5	-0.5	-0.1
Morales et al.	2013	201.167	-62.483	–	–	–	–
Gozha et al.	2012	201.167	-62.483	–	–	–	–
Piskunov et al.	2008	201.15	-62.496	–	–	–	–
Kharchenko et al.	2005	201.16	-62.5	–	-6.45	-0.93	–
Dias et al.	2002	201.167	-62.483	–	-7.55	-3.61	-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]	B_frac	BSS
UCC	99999–	0.93	0.62	–	200	-0.185	56	–	–
Just et al.	2023	–	–	–	200	–	18	–	–
Loktin & Popova	2017	1.47	4.06	–	398	–	–	–	–
Kharchenko et al.	2016	0.70	0.62	–	200	–	–	–	–
Kharchenko et al.	2013	0.70	0.62	–	200	–	–	–	–
Morales et al.	2013	0.93	–	–	200	–	–	–	–
Gozha et al.	2012	0.93	–	–	200	-0.180	95	–	–
Piskunov et al.	2008	0.93	0.62	–	200	–	–	–	–
Kharchenko et al.	2005	0.93	0.62	–	200	–	–	–	–
Dias et al.	2002	0.93	0.62	–	200	-0.190	–	–	–

Visualization

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