UFMG 95

0.37 UTI

0.3

C_N

0.42

C_dens

1.0

C_C3

0.06

C_lit

1.0

C_dup

N_m (P>50%) 30

Core radius and density 1.3 [pc], 2.1 [pc^-2]

C3 classification AA

C_N 0.3 Poorly populated
C_dens 0.42 Loose
C_C3 1.0 Very high quality
C_lit 0.06 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 95 is a poorly populated, loose object of very high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a very metal-poor, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is rarely studied in the literature.

Relatively close Low extinction Very metal-poor Young

Cavallo et al. (2024)
Gold sample.

Hunt & Reffert (2024)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Hunt & Reffert (2023)
Classified as open cluster. CMD class: 1.00 (50th percentile).

Data

🔍 Search references for UFMG 95 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–	270.695	-29.377	0.849	1.808	-0.952	-19.872
Hunt & Reffert	2024	270.688	-29.384	0.845	1.797	-1.017	-17.399
Cavallo et al.	2024	270.665	-29.384	0.845	–	–	–
Hunt & Reffert	2023	270.688	-29.384	0.845	1.797	-1.017	-17.399
Ferreira et al.	2021	270.695	-29.37	0.839	1.815	-0.895	–

💡 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–	1.065	0.36	0.41	57	-1.160	227	–	–
Hunt & Reffert	2024	1.13	0.25	0.41	57	–	227⁽¹⁾	–	–
Cavallo et al.	2024	0.89	1.24	–	35	-1.160	–	–	–
Hunt & Reffert	2023	1.13	0.25	0.41	57	–	–	–	–
Ferreira et al.	2021	1.00	0.47	–	158	–	–	–	–

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

Visualization

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