Majaess 133
0.71
UTI
0.79
CN
1.0
Cdens
1.0
CC3
0.38
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.38 Poorly studied
- Cdup 1.0 Unique
Overview
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.
Very distant
High extinction
Very massive
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 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 | â | â | â |
| 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 | â | -2.15 | -2.27 | â |
| Dias et al. | 2002 | 164.679 | -61.188 | â | -2.15 | -2.27 | 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 | 6004* | â | â |
| Cavallo et al. | 2024 | 3.50 | 3.38 | â | 69 | -0.200 | â | â | â |
| He et al. | 2023 | 10.00 | 4.25 | â | 5 | â | â | â | â |
| Hunt & Reffert | 2023 | 8.32 | 3.02 | 2.83 | 13 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Bronze sample.