UFMG 86

0.03 UTI

0.67

C_N

1.0

C_dens

1.0

C_C3

0.0

C_lit

0.05

C_dup

N₅₀ (P>50% members) 84

Stellar density (N₅₀/rad) 6.2 [N/pc²]

C3 classification AA

C_N 0.67 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.0 Rarely studied
C_dup 0.05 Very likely duplicate

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UFMG 86 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, near the mid-plane, affected by high extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied 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.

(*): The parallax distance estimate (~2.26 kpc) differs significantly from the median photometric distance (~1.45 kpc).

Relatively close High extinction Intermediate age

Data

🔍 Search references for UFMG 86 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–	261.58	-37.794	0.443	0.586	-0.984	-8.601
Ferreira et al.	2021	261.578	-37.8	0.447	0.576	-0.977	–

💡 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–	1.45	3.56	–	224	–	–	–	–
Ferreira et al.	2021	1.45	3.56	–	224	–	–	–	–

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
PHOC 18	95.2	261.59	-37.78	0.44	0.59	-0.98	-8.6	0.65
CWWDL 1647	57.1	261.58	-37.76	0.44	0.57	-0.98	-8.6	0.0

💡 Note: The % column shows the percentage of members that UFMG 86 shares with each listed object.

Visualization

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