UFMG 89

0.64 UTI

0.71

C_N

1.0

C_dens

1.0

C_C3

0.25

C_lit

1.0

C_dup

N₅₀ (P>50% members) 92

Stellar density (N₅₀/rad) 19.0 [N/pc²]

C3 classification AA

C_N 0.71 Moderately populated
C_dens 1.0 Very dense
C_C3 1.0 Very high quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19

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

Overview

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UFMG 89 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate^* distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, young cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.

(*): The parallax distance estimate (~2.70 kpc) differs significantly from the median photometric distance (~1.88 kpc).

Relatively close High extinction Massive Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

🔍 Search references for UFMG 89 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–	269.29	-27.605	0.371	0.298	-1.982	8.885
Hunt & Reffert	2024	269.279	-27.607	0.36	0.309	-2.011	41.108
Cavallo et al.	2024	269.273	-27.608	0.36	–	–	–
Hunt & Reffert	2023	269.279	-27.607	0.36	0.309	-2.011	41.108
Ferreira et al.	2021	269.3	-27.59	0.403	0.29	-1.896	–

💡 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–	1.88	4.1	2.41	21	-0.300	1057	–	–
Hunt & Reffert	2024	–	–	–	–	–	1057⁽¹⁾	–	–
Cavallo et al.	2024	1.88	4.21	–	21	-0.300	–	–	–
Hunt & Reffert	2023	2.55	4.10	2.41	14	–	–	–	–
Ferreira et al.	2021	1.38	3.78	–	316	–	–	–	–

(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.

Visualization

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