ESO 141 47

(MWSC 3085)

0.24 UTI

0.0

C_N

0.05

C_dens

0.25

C_C3

0.44

C_lit

1.0

C_dup

C3 classification CC

Number of members (P>50%) 20

Radius (P>50% members) 7.2 [arcmin]

C_N 0.0 Sparse
C_dens 0.05 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 141 47 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate^* distance, well below the mid-plane, affected by low extinction. It is catalogued as a massive, old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~4.20 kpc) differs significantly from the median photometric distance (~2.63 kpc).

Relatively close Low extinction Massive Old

Data

🔍 Search references for ESO 141 47 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	–	289.478	-57.895	0.238	-0.809	-5.295	26.539
Just et al.	2023	289.552	-57.902	–	–	–	–
Bica et al.	2019	289.507	-57.904	–	–	–	–
Loktin & Popova	2017	289.515	-57.903	–	4.571	-8.606	-23.5
Kharchenko et al.	2016	289.552	-57.902	–	–	–	–
Dias et al.	2014	289.512	-57.903	–	3.48	-6.46	-23.5
Kharchenko et al.	2013	289.563	-57.9	–	7.34	-6.29	–
Dias et al.	2002	289.512	-57.903	–	2.9	-7.89	-23.5

💡 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	–	–	–	2786	–	1021	–	–
Loktin & Popova	2017	2.29	0.55	–	6310	–	–	–	–
Kharchenko et al.	2016	2.97	0.32	–	2786	–	–	–	–
Kharchenko et al.	2013	2.97	0.32	–	2786	–	–	–	–
Dias et al.	2002	1.79	1.02	–	1259	–	–	–	–

Visualization

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