ESO 525 08

(MWSC 3125)

0.21 UTI

0.0

C_N

0.04

C_dens

0.12

C_C3

0.44

C_lit

1.0

C_dup

C3 classification DC

Number of members (P>50%) 20

Radius (P>50% members) 4.7 [arcmin]

C_N 0.0 Sparse
C_dens 0.04 Very loose
C_C3 0.12 Very 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

ℹ️

ESO 525 08 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a large^* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an old cluster (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~7.73 kpc) differs significantly from the median photometric distance (~2.46 kpc).

Relatively close Moderate extinction Old

Data

🔍 Search references for ESO 525 08 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	291.844	-23.576	0.129	-2.517	-4.297	144.67
Just et al.	2023	291.787	-23.592	–	–	–	–
Bica et al.	2019	291.821	-23.587	–	–	–	–
Loktin & Popova	2017	291.84	-23.619	–	1.749	-1.889	–
Kharchenko et al.	2016	291.787	-23.592	–	–	–	–
Dias et al.	2014	291.817	-23.576	–	0.99	-1.43	–
Kharchenko et al.	2013	291.795	-23.59	–	-0.14	-1.58	–
Dias et al.	2002	291.817	-23.576	–	0.99	-1.43	–

💡 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	–	–	–	1585	–	861	–	–
Loktin & Popova	2017	2.36	0.14	–	1820	–	–	–	–
Kharchenko et al.	2016	2.57	1.48	–	1585	–	–	–	–
Kharchenko et al.	2013	2.57	1.48	–	1585	–	–	–	–
Dias et al.	2002	1.64	1.12	–	1000	–	–	–	–

Visualization

ℹ️