UFMG 11

0.55 UTI

0.76

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 140

Stellar density (N₅₀/rad) 14.0 [N/pc²]

C3 classification AA

C_N 0.76 Rich
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UFMG 11 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature, with no articles listed in the last 6 years.

(*): The parallax distance estimate (~3.29 kpc) differs significantly from the median photometric distance (~2.46 kpc).

Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.

Relatively close Moderate extinction Intermediate age

Data

🔍 Search references for UFMG 11 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–	243.505	-52.959	0.304	-2.082	-1.9	-25.516
Ferreira et al.	2020	243.5	-52.963	0.3	-2.083	-2.05	–

💡 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–	2.46	2.08	–	251	–	–	–	–
Ferreira et al.	2020	2.46	2.08	–	251	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
UBC 1543	85.7	243.51	-52.96	0.31	-2.08	-1.87	-26.02	0.16
Theia 3669	83.6	243.5	-52.96	0.31	-2.08	-1.87	-25.52	0.02

💡 Note: The % column shows the percentage of members that UFMG 11 shares with each listed object.

Visualization

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