Lynga 13

(MWSC 2468)

0.17 UTI

0.0

C_N

0.03

C_dens

0.12

C_C3

0.35

C_lit

1.0

C_dup

N₅₀ (P>50% members) 11

Stellar density (N₅₀/rad) 0.1 [N/pc²]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.03 Very loose
C_C3 0.12 Very low quality
C_lit 0.35 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Lynga 13 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is poorly 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.

Distant High extinction Near-solar metallicity Old

Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.

Data

🔍 Search references for Lynga 13 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–	252.214	-43.423	0.237	-2.805	-4.713	–
Just et al.	2023	252.222	-43.428	–	–	–	–
Kharchenko et al.	2016	252.222	-43.428	–	–	–	–
Dias et al.	2014	252.221	-43.433	–	-1.71	-2.25	–
Kharchenko et al.	2013	252.232	-43.428	–	-6.77	-1.59	–
Morales et al.	2013	252.221	-43.433	–	–	–	–
Dias et al.	2002	252.221	-43.433	–	-1.71	-2.25	–

💡 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–	3.41	3.23	–	1585	0.000	161	–	–
Just et al.	2023	–	–	–	1585	–	161	–	–
Kharchenko et al.	2016	3.41	3.23	–	1585	–	–	–	–
Kharchenko et al.	2013	3.41	3.23	–	1585	–	–	–	–
Dias et al.	2002	1.14	1.58	–	832	0.000	–	–	–

Visualization

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