Dias 32

0.16 UTI

0.42

C_N

0.63

C_dens

0.5

C_C3

0.0

C_lit

0.52

C_dup

N₅₀ (P>50% members) 42

Stellar density (N₅₀/rad) 3.1 [N/pc²]

C3 classification BB

C_N 0.42 Poorly populated
C_dens 0.63 Moderately dense
C_C3 0.5 Intermediate quality
C_lit 0.0 Rarely studied
C_dup 0.52 Likely unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

ℹ️

Dias 32 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It was recently reported in the literature.

Note: This is likely a unique object, which shares a moderate percentage of members with at least one previously reported entry. See table with shared members information.

Distant High extinction Near-solar metallicity Intermediate age

Data

🔍 Search references for Dias 32 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	99999–	278.275	-11.908	0.294	-0.282	-1.813	2.147
Dias & Monteiro	2025	278.298	-11.905	0.261	-0.304	-1.854	5.205

💡 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–	4.78	4.05	–	665	0.332	–	–	–
Dias & Monteiro	2025	4.78	4.05	–	665	0.332	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 3154	47.6	278.27	-11.91	0.19	-0.2	-1.72	52.75	0.46

💡 Note: The % column shows the percentage of members that Dias 32 shares with each listed object.

Visualization

ℹ️