ESO 311 14

(MWSC 1352)

0.23 UTI

0.0

C_N

0.01

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 13

Radius (P>50% members) 7.6 [arcmin]

C_N 0.0 Sparse
C_dens 0.01 Very loose
C_C3 0.25 Low quality
C_lit 0.44 Poorly studied
C_dup 1.0 Unique

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

Overview

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ESO 311 14 is a sparse, very loose object of low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by low extinction. It is catalogued as a low-mass, young cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~6.44 kpc) differs significantly from the median photometric distance (~1.45 kpc).

Relatively close Low extinction Low mass Young

Data

🔍 Search references for ESO 311 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	–	117.36	-42.679	0.155	-2.096	2.843	59.196
Just et al.	2023	117.345	-42.682	–	–	–	–
Bica et al.	2019	117.348	-42.697	–	–	–	–
Loktin & Popova	2017	117.345	-42.685	–	-3.012	5.429	–
Kharchenko et al.	2016	117.345	-42.682	–	–	–	–
Dias et al.	2014	117.35	-42.705	–	-5.12	2.33	–
Kharchenko et al.	2013	117.349	-42.685	–	-1.12	5.58	–
Dias et al.	2002	117.35	-42.705	–	-5.86	3.15	–

💡 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
Just et al.	2023	–	–	–	55	–	31	–	–
Loktin & Popova	2017	3.62	0.85	–	398	–	–	–	–
Kharchenko et al.	2016	1.28	0.64	–	55	–	–	–	–
Kharchenko et al.	2013	1.28	0.64	–	55	–	–	–	–
Dias et al.	2002	1.61	0.31	–	1000	–	–	–	–

Visualization

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