Majaess 90

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0.52 UTI
0.34
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad) 7.5 [N/pc2]
  • CN 0.34 Poorly populated
  • Cdens 1.0 Very dense
  • CC3 0.75 High quality
  • Clit 0.25 Poorly studied
  • Cdup 1.0 Unique

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, but with a large variance across recent sources for the age parameter (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.

Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P234, along with Ivanov_6.

Cavallo et al. (2024)
Bronze sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC 99999– 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] Bfrac BSS
UCC 99999– 1.315 1.61 2.03 116 0.240 100 – –
Hunt & Reffert 2024 – – – – – 100(1) – –
Cavallo et al. 2024 1.31 1.08 – 219 0.240 – – –
Hunt & Reffert 2023 1.32 2.14 2.03 12 – – – –

(N): Indicates that there are N extra values assigned to this parameter 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 0.69

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

Visualization

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