Theia 3932

0.01 UTI

0.37

C_N

0.3

C_dens

0.75

C_C3

0.0

C_lit

0.03

C_dup

C3 classification AB

Number of members (P>50%) 37

Radius (P>50% members) 13.9 [arcmin]

C_N 0.37 Poorly populated
C_dens 0.3 Loose
C_C3 0.75 High quality
C_lit 0.0 Rarely studied
C_dup 0.03 Very likely duplicate

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

Overview

ℹ️

Theia 3932 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a relatively close 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 very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for Theia 3932 in: SciX Simbad

ℹ️

Reference	Year	RA [deg]	DEC [deg]	Plx [mas]	pmRA [mas/yr]	pmDE [mas/yr]	Rv [km/s]
UCC	–	119.319	-35.137	0.809	-4.652	2.238	27.482
Hunt & Reffert	2024	119.275	-35.191	0.79	-4.621	2.235	28.674
Cavallo et al.	2024	119.383	-35.098	0.79	–	–	–
Hunt & Reffert	2023	119.275	-35.191	0.79	-4.621	2.235	28.674

💡 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
Hunt & Reffert	2024	–	–	–	–	–	132*	–	–
Cavallo et al.	2024	1.25	1.64	–	174	0.020	–	–	–
Hunt & Reffert	2023	1.19	1.35	0.95	260	–	–	–	–

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

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Casado 5	97.3	119.37	-35.1	0.8	-4.65	2.23	22.28	0.38

💡 Note: The % column shows the percentage of members that Theia 3932 shares with each listed object.

Visualization

ℹ️

1 2