Majaess 99

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0.60 UTI
0.75
CN
1.0
Cdens
0.5
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members) 7.3 [arcmin]
  • CN 0.75 Rich
  • Cdens 1.0 Very dense
  • CC3 0.5 Intermediate quality
  • Clit 0.38 Poorly studied
  • Cdup 1.0 Unique

Overview

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Majaess 99 is a rich, very dense object of intermediate 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, very young cluster (see Parameters). It is poorly studied in the literature.

Note: This object shares a moderate percentage of members with 3 later reported entries. See table with shared members information.

Relatively close Moderate extinction Near-solar metallicity Very young

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 – 125.539 -42.103 0.66 -4.335 5.247 0.76
Hunt & Reffert 2024 125.489 -42.084 0.66 -4.344 5.232 10.996
Cavallo et al. 2024 125.616 -42.128 0.663 – – –
Hunt & Reffert 2023 125.489 -42.084 0.66 -4.344 5.232 10.996
Monteiro & Dias 2019 125.438 -42.082 – -4.372 5.187 2.308
Dias et al. 2014 125.438 -42.082 – -4.29 2.62 –
Dias et al. 2002 125.438 -42.082 – -4.51 1.54 –

💡 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 – – – – – 396* – –
Cavallo et al. 2024 1.40 1.43 – 59 0.350 – – –
Hunt & Reffert 2023 1.45 1.80 2.71 6 – – – –
Monteiro & Dias 2019 1.32 0.06 – 5 0.012 – – –

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

Cluster % RA DEC Plx pmRA pmDE Rv UTI
CWWDL 13331 44.5 125.54 -42.12 0.66 -4.31 5.28 -7.14 0.0
OC 0463 38.2 125.49 -42.1 0.66 -4.32 5.2 0.76 0.0
OC 0466 30.0 125.65 -42.12 0.66 -4.31 5.31 0.76 0.01

💡 Note: The % column shows the percentage of members that Majaess 99 shares with each listed object.

Visualization

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