Dias 24

0.02 UTI

0.0

C_N

0.2

C_dens

0.5

C_C3

0.0

C_lit

0.16

C_dup

N₅₀ (P>50% members) 22

Stellar density (N₅₀/rad) 1.0 [N/pc²]

C3 classification BB

C_N 0.0 Sparse
C_dens 0.2 Very loose
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.16 Likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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Dias 24 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a large distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

⚠️ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Very distant Moderate extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for Dias 24 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–	122.866	-34.078	0.166	-2.474	3.009	66.426
Dias & Monteiro	2025	122.878	-34.075	0.167	-2.482	3.008	96.46

💡 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–	5.77	1.68	–	151	-0.194	–	–	–
Dias & Monteiro	2025	5.77	1.68	–	151	-0.194	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3656	84.0	122.87	-34.07	0.18	-2.49	3.01	45.64	0.15

💡 Note: The % column shows the percentage of members that Dias 24 shares with each listed object.

Visualization

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