Theia 2227
0.10
UTI
0.46
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.22
Cdup
Stellar density (N50/rad)
25.8 [N/pc2]
- CN 0.46 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.22 Likely duplicate
Overview
Theia 2227 is a poorly populated, very dense object of high 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, intermediate-age cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 235.0 | -58.487 | 0.566 | -2.175 | -3.549 | â |
| Hunt & Reffert | 2024 | 235.019 | -58.489 | 0.555 | -2.187 | -3.564 | â |
| Cavallo et al. | 2024 | 234.987 | -58.48 | 0.558 | â | â | â |
| Hunt & Reffert | 2023 | 235.019 | -58.489 | 0.555 | -2.187 | -3.564 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.7 | 1.86 | 0.37 | 109 | 0.380 | 235 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 235(1) | â | â |
| Cavallo et al. | 2024 | 1.71 | 2.00 | â | 135 | 0.380 | â | â | â |
| Hunt & Reffert | 2023 | 1.69 | 1.72 | 0.37 | 83 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.