UFMG 29

0.60 UTI

0.76

C_N

1.0

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 135

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

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

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

Overview

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UFMG 29 is a rich, very dense 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 is poorly studied in the literature.

Note: This object shares a significant percentage of members with a later reported entry. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit.

Data

🔍 Search references for UFMG 29 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	–	258.814	-36.581	0.635	-1.028	0.521	-31.289
Li et al.	2025	258.818	-36.582	0.584	-0.978	0.522	–
Almeida et al.	2025	258.818	-36.582	–	–	–	–
Dias et al.	2021	258.818	-36.582	0.584	-0.978	0.522	–
Ferreira et al.	2020	258.834	-36.603	0.585	-0.986	0.524	–

💡 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
Li et al.	2025	1.31	2.17	–	631	-0.130	–	–	–
Almeida et al.	2025	1.56	2.35	–	222	–	138	–	–
Dias et al.	2021	1.56	2.35	–	222	0.082	–	–	–
Ferreira et al.	2020	1.38	2.39	–	501	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1777	65.9	258.81	-36.57	0.63	-1.03	0.52	-31.29	0.0

💡 Note: The % column shows the percentage of members that UFMG 29 shares with each listed object.

Visualization

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