Majaess 133

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0.70 UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad) 6.2 [N/pc2]
  • CN 0.79 Rich
  • Cdens 1.0 Very dense
  • CC3 1.0 Very high quality
  • Clit 0.35 Poorly studied
  • Cdup 1.0 Unique

Overview

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Majaess 133 is a rich, very dense object of very high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a very massive, near-solar metallicity, very young 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 a later reported entry. See table with shared members information.

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– 164.66 -61.182 0.111 -5.524 2.295 32.404
Hunt & Reffert 2024 164.67 -61.18 0.114 -5.546 2.298 56.801
Cavallo et al. 2024 164.654 -61.186 0.115 – – –
He et al. 2023 164.664 -61.182 0.108 -5.486 2.302 32.4
Hunt & Reffert 2023 164.67 -61.18 0.114 -5.546 2.298 56.801
Dias et al. 2014 164.679 -61.188 – -2.15 -2.27 –
Dias et al. 2002 164.679 -61.188 – -2.15 -2.27 –

💡 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– 8.32 3.38 2.83 13 -0.200 6004 – –
Hunt & Reffert 2024 – – – – – 6004(1) – –
Cavallo et al. 2024 3.50 3.38 – 69 -0.200 – – –
He et al. 2023 10.00 4.25 – 5 – – – –
Hunt & Reffert 2023 8.32 3.02 2.83 13 – – – –

(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 3854 2.9 164.7 -60.98 0.17 -5.59 2.24 – 0.08

💡 Note: The % column shows the percentage of members that Majaess 133 shares with each listed object.

Visualization

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