Theia 3167
0.22
UTI
0.0
CN
0.33
Cdens
0.75
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
7.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.33 Loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 3167 is a sparse, loose object of high C3 quality. Its parallax locates it at a relatively close distance, near 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: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 212.152 | -63.509 | 0.584 | -7.819 | -2.234 | -29.651 |
| Hunt & Reffert | 2024 | 212.118 | -63.522 | 0.573 | -7.795 | -2.231 | -37.192 |
| Cavallo et al. | 2024 | 212.211 | -63.517 | 0.579 | â | â | â |
| Hunt & Reffert | 2023 | 212.118 | -63.522 | 0.573 | -7.795 | -2.231 | -37.192 |
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 | 117* | â | â |
| Cavallo et al. | 2024 | 1.44 | 1.14 | â | 407 | 0.030 | â | â | â |
| Hunt & Reffert | 2023 | 1.63 | 0.96 | 0.25 | 217 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.