Majaess 90

0.52 UTI

0.34

C_N

1.0

C_dens

0.75

C_C3

0.25

C_lit

1.0

C_dup

C3 classification AB

Number of members (P>50%) 34

Radius (P>50% members) 5.4 [arcmin]

C_N 0.34 Poorly populated
C_dens 1.0 Very dense
C_C3 0.75 High quality
C_lit 0.25 Poorly studied
C_dup 1.0 Unique

📥 Members 📊 Colab 🔬 Bayestar19 🔍 CDS 🔍 Simbad 🔍 CDS (α, δ) 🔍 Simbad (α, δ)

Overview

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Majaess 90 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Intermediate age

Cavallo et al. (2024)
Bronze sample.

Data

🔍 Search references for Majaess 90 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	–	111.185	-24.484	0.738	-2.156	2.268	31.616
Hunt & Reffert	2024	111.206	-24.505	0.742	-2.158	2.267	26.991
Cavallo et al.	2024	111.031	-24.379	0.74	–	–	–
Hunt & Reffert	2023	111.206	-24.505	0.742	-2.158	2.267	26.991
Dias et al.	2002	111.188	-24.493	–	-6.54	22.43	–

💡 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]	Bfr	BSS
Hunt & Reffert	2024	–	–	–	–	–	100*	–	–
Cavallo et al.	2024	1.31	1.08	–	219	0.240	–	–	–
Hunt & Reffert	2023	1.32	2.14	2.03	12	–	–	–	–

(*): Indicates that this parameter is assigned more than one value in the corresponding reference.

Cluster	%	RA	DEC	Plx	pmRA	pmDE	Rv	UTI
CWNU 1337	76.5	111.03	-24.4	0.72	-2.14	2.23	31.62	0.18
Ivanov 6	5.9	111.06	-24.64	0.72	-2.05	2.69	18.64	0.67

💡 Note: The % column shows the percentage of members that Majaess 90 shares with each listed object.

Visualization

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