Lynga 14

(OCL 992; ESO 277 18; MWSC 2484)

UTI: UCC Trust Index C_N C_dens C_C3 C_lit C_dup 0.64 1.0 1.0 0.79 1.0
C3	N_50	r_50
AA	78	3.8

Summary

Lynga 14 is a moderately populated, very dense object of very high C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is well-studied in the literature.

This object shares a large percentage of members with a later reported entry.

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Positions

Reference	RA	DEC	Plx	pmRA	pmDE	Rv
Dambis (1999)	253.75	-45.333	–	–	–	–
Dias et al. (2002)	253.767	-45.233	–	0.79	-2.8	–
Kharchenko et al. (2012)	253.748	-45.24	–	-1.8	-1.48	–
Loktin & Popova (2017)	253.77	-45.234	–	-3.499	-0.703	–
Cantat-Gaudin et al. (2018)	253.764	-45.239	0.308	-0.336	-1.977	–
Bica et al. (2019)	253.76	-45.241	–	–	–	–
Cantat-Gaudin et al. (2020)	253.764	-45.239	0.308	-0.336	-1.977	–
Hunt & Reffert (2023)	253.766	-45.236	0.36	-0.427	-1.996	-61.17
Cavallo et al. (2024)	253.741	-45.224	0.359	–	–	–
Hunt & Reffert (2024)	253.766	-45.236	0.36	-0.427	-1.996	-61.17
UCC	253.763	-45.233	0.354	-0.385	-1.986	-51.809

Galactocentric position

How are the galactocentric plots generated?

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Estimated members

1 2 3

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Fundamental parameters

Reference	Values
Dambis (1999)	E_B-V_=1.483, DM0=11.84, log_age_=6.4
Dias et al. (2002)	E(B-V)=1.428, Dist=881.0, Age=6.712
Kharchenko et al. (2012)	e_bv=1.197, distance=1327, log_age=7.75
Loktin & Popova (2017)	E(B-V)=1.305, Dist=950, logt=7.057
Cantat-Gaudin et al. (2018)	dmode=2963.2
Hunt & Reffert (2023)	AV50=3.454, diffAV50=2.941, MOD50=12.003, logAge50=6.815
Cavallo et al. (2024)	AV50=3.56, dMod50=12.25, logAge50=7.25, [Fe/H]50=0.81
Hunt & Reffert (2024)	MassJ=2175.11, MassTot=2221.78

Search coordinates in Bayestar19

Cluster region map

Objects with shared members

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