Theia 817
0.18
UTI
0.26
CN
0.41
Cdens
0.25
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
33.5 [arcmin]
- CN 0.26 Poorly populated
- Cdens 0.41 Loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 817 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a very close distance, above the mid-plane, affected by low 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.
Very close
Low 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 | 274.892 | 24.55 | 2.744 | -2.015 | 1.194 | -25.032 |
| Zhang et al. | 2024 | 274.95 | 24.606 | â | â | â | â |
| Cavallo et al. | 2024 | 274.738 | 24.266 | 2.732 | â | â | â |
| Hunt & Reffert | 2023 | 274.95 | 24.606 | 2.757 | -2.018 | 1.299 | -22.438 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.125* | â | â | â |
| Cavallo et al. | 2024 | 0.38 | 0.60 | â | 251 | 0.390 | â | â | â |
| Hunt & Reffert | 2023 | 0.35 | 0.25 | 0.71 | 195 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.