UFMG 72

0.48 UTI

0.45

C_N

0.96

C_dens

1.0

C_C3

0.0

C_lit

1.0

C_dup

N₅₀ (P>50% members) 45

Stellar density (N₅₀/rad) 4.8 [N/pc²]

C3 classification AA

C_N 0.45 Poorly populated
C_dens 0.96 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 72 is a poorly populated, very dense object of very high C3 quality. Its parallax locates it at a relatively close^* distance, near the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.

(*): The parallax distance estimate (~1.41 kpc) differs significantly from the median photometric distance (~1.05 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 72 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–	268.532	-23.129	0.711	0.08	-2.609	-10.551
Ferreira et al.	2021	268.515	-23.17	0.686	0.096	-2.569	–

💡 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–	1.05	2.33	–	126	–	–	–	–
Ferreira et al.	2021	1.05	2.33	–	126	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
Theia 1761	91.1	268.6	-23.09	0.71	0.08	-2.61	-5.4	0.06
CWWDL 14199	86.7	268.6	-23.09	0.71	0.08	-2.61	0.14	0.14

💡 Note: The % column shows the percentage of members that UFMG 72 shares with each listed object.

Visualization

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