Majaess 225

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0.45 UTI
0.52
CN
0.38
Cdens
0.5
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members) 5.8 [arcmin]
  • CN 0.52 Moderately populated
  • Cdens 0.38 Loose
  • CC3 0.5 Intermediate quality
  • Clit 0.44 Poorly studied
  • Cdup 1.0 Unique

Overview

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Majaess 225 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, young cluster (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.

Distant High extinction Near-solar metallicity Young

Cavallo et al. (2024)
Gold sample.

Data

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Reference Year RA [deg] DEC [deg] Plx [mas] pmRA [mas/yr] pmDE [mas/yr] Rv [km/s]
UCC – 354.773 61.948 0.316 -3.467 -1.666 –
Hunt & Reffert 2024 354.786 61.92 0.319 -3.442 -1.678 –
Cavallo et al. 2024 354.767 61.969 0.319 – – –
He et al. 2023 354.733 62.056 0.322 -3.389 -1.682 –
Hunt & Reffert 2023 354.786 61.92 0.319 -3.442 -1.678 –
Monteiro & Dias 2019 354.933 61.93 – -3.629 -1.405 2.255
Dias et al. 2014 354.95 61.928 – -2.01 -2.59 -57.0
Dias et al. 2002 354.95 61.928 – -2.01 -2.59 -57.0

💡 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 – – – – – 524* – –
Cavallo et al. 2024 3.15 2.89 – 39 0.450 – – –
He et al. 2023 2.88 3.35 – 16 – – – –
Hunt & Reffert 2023 2.84 2.93 1.79 28 – – – –
Monteiro & Dias 2019 3.60 3.11 – 11 0.016 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
BDSB 46 1.9 354.94 61.93 0.49 -3.61 -1.39 -48.33 0.4

💡 Note: The % column shows the percentage of members that Majaess 225 shares with each listed object.

Visualization

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