Lynga 14

(MWSC 2484; OCL 992; ESO 277 18)

0.85 UTI

0.64

C_N

1.0

C_dens

1.0

C_C3

0.81

C_lit

1.0

C_dup

N₅₀ (P>50% members) 78

Stellar density (N₅₀/rad) 8.0 [N/pc²]

C3 classification AA

C_N 0.64 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.81 Well-studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Lynga 14 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, very young cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.

(*): The parallax distance estimate (~2.83 kpc) differs significantly from the median photometric distance (~1.83 kpc).

Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.

Relatively close High extinction Massive Metal-rich Very young

Cavallo et al. (2024)
Bronze sample.

Data

🔍 Search references for Lynga 14 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–	253.763	-45.233	0.354	-0.385	-1.986	-51.809
Hunt & Reffert	2024	253.766	-45.236	0.36	-0.427	-1.996	-61.17
Cavallo et al.	2024	253.741	-45.224	0.359	–	–	–
Hunt & Reffert	2023	253.766	-45.236	0.36	-0.427	-1.996	-61.17
Just et al.	2023	253.737	-45.239	–	–	–	–
Cantat-Gaudin et al.	2020	253.764	-45.239	0.308	-0.336	-1.977	–
Cantat-Gaudin & Anders	2020	253.764	-45.239	0.308	-0.336	-1.977	–
Bica et al.	2019	253.76	-45.241	–	–	–	–
Cantat-Gaudin et al.	2018	253.764	-45.239	0.308	-0.336	-1.977	–
Loktin & Popova	2017	253.77	-45.234	–	-3.499	-0.703	–
Kharchenko et al.	2016	253.737	-45.239	–	–	–	–
Dias et al.	2014	253.767	-45.233	–	0.79	-2.8	–
Kharchenko et al.	2013	253.747	-45.24	–	-1.8	-1.48	–
van den Bergh	2006	253.753	-45.333	–	–	–	–
Dias et al.	2002	253.767	-45.233	–	0.79	-2.8	–
Dambis	1999	253.75	-45.333	–	–	–	–

💡 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–	1.83	3.88	2.94	11	0.810	1102	–	–
Hunt & Reffert	2024	–	–	–	–	–	2175⁽¹⁾	–	–
Cavallo et al.	2024	2.82	3.56	–	18	0.810	–	–	–
Hunt & Reffert	2023	2.52	3.45	2.94	7	–	–	–	–
Just et al.	2023	–	–	–	56	–	29	–	–
Cantat-Gaudin & Anders	2020	2.96	–	–	–	–	–	–	–
Cantat-Gaudin et al.	2018	2.96	–	–	–	–	–	–	–
Loktin & Popova	2017	0.95	4.05	–	11	–	–	–	–
Kharchenko et al.	2016	1.33	3.71	–	56	–	–	–	–
Kharchenko et al.	2013	1.33	3.71	–	56	–	–	–	–
van den Bergh	2006	0.88	4.43	–	5	–	–	–	–
Dias et al.	2002	0.88	4.43	–	5	–	–	–	–
Dambis	1999	2.33	4.60	–	3	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
OC 0670	80.8	253.76	-45.23	0.36	-0.41	-2.0	–	0.05

💡 Note: The % column shows the percentage of members that Lynga 14 shares with each listed object.

Visualization

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