ESO 260 17

(MWSC 1624)

0.31 UTI

0.28

C_N

0.41

C_dens

0.12

C_C3

0.38

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 28

Radius (P>50% members) 4.3 [arcmin]

C_N 0.28 Poorly populated
C_dens 0.41 Loose
C_C3 0.12 Very low quality
C_lit 0.38 Poorly studied
C_dup 1.0 Unique

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

Overview

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ESO 260 17 is a poorly populated, loose object of very low C3 quality. Its parallax locates it at a moderate^* distance, above the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.97 kpc) differs significantly from the median photometric distance (~1.81 kpc).

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for ESO 260 17 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	–	136.241	-46.049	0.337	-3.385	3.503	11.306
Just et al.	2023	136.183	-46.032	–	–	–	–
Bica et al.	2019	136.206	-46.043	–	–	–	–
Kharchenko et al.	2016	136.183	-46.032	–	–	–	–
Dias et al.	2014	136.204	-46.042	–	0.15	4.14	–
Kharchenko et al.	2013	136.188	-46.035	–	-5.68	6.0	–
Dias et al.	2002	136.204	-46.042	–	0.15	4.14	–

💡 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	–	–	–	977	–	56	–	–
Kharchenko et al.	2016	1.81	2.06	–	977	–	–	–	–
Kharchenko et al.	2013	1.81	2.06	–	977	–	–	–	–
Dias et al.	2002	1.37	2.79	–	71	–	–	–	–

Visualization

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