ESO 130 13

(FSR 1612; MWSC 2021; MWSC 2022; FoF 423)

0.95 UTI

0.77

C_N

1.0

C_dens

1.0

C_C3

1.0

C_lit

1.0

C_dup

C3 classification AA

Number of members (P>50%) 157

Radius (P>50% members) 3.1 [arcmin]

C_N 0.77 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 1.0 Very well-studied
C_dup 1.0 Unique

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

Overview

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ESO 130 13 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.

Relatively close Moderate extinction Near-solar metallicity Young

Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for ESO 130 13 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	–	185.764	-59.643	0.383	-4.423	-0.394	-15.85
Li et al.	2025	185.782	-59.644	0.386	-4.422	-0.417	–
Almeida et al.	2025	185.802	-59.651	–	–	–	–
Hunt & Reffert	2024	185.779	-59.657	0.392	-4.426	-0.39	-28.722
Cavallo et al.	2024	185.785	-59.643	0.393	–	–	–
Hunt & Reffert	2023	185.779	-59.657	0.392	-4.426	-0.39	-28.722
Almeida et al.	2023	185.791	-59.649	–	–	–	–
Just et al.	2023	185.758	-59.662	–	–	–	–
Dias et al.	2021	185.802	-59.651	0.395	-4.421	-0.397	-6.423
Cantat-Gaudin et al.	2020	185.782	-59.644	0.386	-4.422	-0.417	–
Sánchez et al.	2020	185.825	-59.66	–	-4.419	-0.37	–
Cantat-Gaudin & Anders	2020	185.782	-59.644	0.386	-4.422	-0.417	–
Liu & Pang	2019	185.792	-59.645	0.398	-4.432	-0.419	–
Bica et al.	2019	185.825	-59.658	–	–	–	–
Cantat-Gaudin et al.	2018	185.782	-59.644	0.386	-4.422	-0.417	–
Kharchenko et al.	2016	185.758	-59.662	–	–	–	–
Dias et al.	2014	185.825	-59.66	–	-3.62	-0.9	–
Kharchenko et al.	2013	185.767	-59.665	–	-7.53	-4.45	–
Froebrich et al.	2007	185.842	-59.631	–	–	–	–
Dias et al.	2002	185.825	-59.66	–	-3.62	-0.9	–

💡 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
Li et al.	2025	2.00	1.50	–	95	-0.240	–	–	–
Almeida et al.	2025	2.14	1.60	–	52	–	505	–	–
Hunt & Reffert	2024	–	–	–	–	–	860*	–	–
Cavallo et al.	2024	2.17	1.67	–	56	-0.070	–	–	–
Hunt & Reffert	2023	2.33	1.41	1.12	89	–	–	–	–
Almeida et al.	2023	2.20	1.62	–	53	0.068	607*	0.59	–
Just et al.	2023	–	–	–	279	–	193	–	–
Dias et al.	2021	2.14	1.60	–	52	0.024	–	–	–
Cantat-Gaudin et al.	2020	2.42	1.38	–	34	–	–	–	–
Cantat-Gaudin & Anders	2020	2.41	–	–	–	–	–	–	–
Liu & Pang	2019	–	–	–	34	0.250	–	–	–
Cantat-Gaudin et al.	2018	2.41	–	–	–	–	–	–	–
Kharchenko et al.	2016	1.51	1.03	–	279	–	–	–	–
Kharchenko et al.	2013	1.51	1.03	–	279	–	–	–	–
Dias et al.	2002	4.32	1.95	–	1259	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Visualization

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