ESO 132 14

0.13 UTI

0.0

C_N

0.28

C_dens

0.12

C_C3

0.13

C_lit

1.0

C_dup

N_m (P>50%) 24

Core radius and density 0.8 [pc], 1.4 [pc^-2]

C3 classification DC

C_N 0.0 Sparse
C_dens 0.28 Loose
C_C3 0.12 Very low quality
C_lit 0.13 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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ESO 132 14 is a sparse, loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by low extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 8 years.

(*): The parallax distance estimate (~2.65 kpc) differs significantly from the median photometric distance (~1.10 kpc).

⚠️ 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.

Relatively close Low extinction Intermediate age

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 ESO 132 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–	204.124	-62.189	0.377	-10.249	-2.073	-41.454
Dias et al.	2018	–	–	–	-7.49	-2.77	–
Dib et al.	2018	204.135	-62.19	–	–	–	–
Sampedro et al.	2017	204.125	-62.214	–	-0.6	-4.23	–
Dias et al.	2014	204.125	-62.214	–	-2.9	-5.14	–
Morales et al.	2013	204.125	-62.214	–	–	–	–
Dias et al.	2002	204.125	-62.214	–	-2.87	-5.23	–

💡 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–	1.1	0.0	–	800	–	–	–	–
Dib et al.	2018	1.09	–	–	1413	–	–	–	–
Morales et al.	2013	1.10	–	–	800	–	–	–	–
Dias et al.	2002	1.10	0.00	–	794	–	–	–	–

Visualization

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