Majaess 88
0.59
UTI
0.7
CN
1.0
Cdens
0.75
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
9.3 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Majaess 88 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low 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 large percentage of members with a later reported entry. See table with shared members information.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 110.979 | -25.87 | 0.762 | -2.672 | 3.285 | 38.552 |
| Hunt & Reffert | 2024 | 110.988 | -25.887 | 0.765 | -2.666 | 3.288 | 34.149 |
| Cavallo et al. | 2024 | 110.949 | -25.778 | 0.763 | â | â | â |
| Hunt & Reffert | 2023 | 110.988 | -25.887 | 0.765 | -2.666 | 3.288 | 34.149 |
| Dias et al. | 2002 | 111.029 | -25.899 | â | -7.28 | 15.9 | â |
đĄ 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 | â | â | â | â | â | 132* | â | â |
| Cavallo et al. | 2024 | 1.40 | 0.63 | â | 17 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 1.25 | 0.74 | 1.42 | 35 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Silver sample.