Majaess 225
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
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
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 354.773 | 61.948 | 0.316 | -3.467 | -1.666 | â |
| Hunt & Reffert | 2024 | 354.786 | 61.92 | 0.319 | -3.442 | -1.678 | â |
| Cavallo et al. | 2024 | 354.767 | 61.969 | 0.319 | â | â | â |
| He et al. | 2023 | 354.733 | 62.056 | 0.322 | -3.389 | -1.682 | â |
| Hunt & Reffert | 2023 | 354.786 | 61.92 | 0.319 | -3.442 | -1.678 | â |
| Monteiro & Dias | 2019 | 354.933 | 61.93 | â | -3.629 | -1.405 | 2.255 |
| Dias et al. | 2014 | 354.95 | 61.928 | â | -2.01 | -2.59 | -57.0 |
| Dias et al. | 2002 | 354.95 | 61.928 | â | -2.01 | -2.59 | -57.0 |
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 | 524* | â | â |
| Cavallo et al. | 2024 | 3.15 | 2.89 | â | 39 | 0.450 | â | â | â |
| He et al. | 2023 | 2.88 | 3.35 | â | 16 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.84 | 2.93 | 1.79 | 28 | â | â | â | â |
| Monteiro & Dias | 2019 | 3.60 | 3.11 | â | 11 | 0.016 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.