Theia 696
0.09
UTI
0.27
CN
0.43
Cdens
0.25
CC3
0.0
Clit
0.48
Cdup
Radius (P>50% members)
41.2 [arcmin]
- CN 0.27 Poorly populated
- Cdens 0.43 Loose
- CC3 0.25 Low quality
- Clit 0.0 Rarely studied
- Cdup 0.48 Possibly duplicate
Overview
Theia 696 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a very close distance, below 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: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry. See table with shared members information.
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 | 272.251 | -73.605 | 3.376 | 1.427 | -14.676 | 20.297 |
| Cavallo et al. | 2024 | 272.784 | -73.828 | 3.466 | â | â | â |
| Hunt & Reffert | 2023 | 271.719 | -73.993 | 3.459 | 1.344 | -14.992 | 15.632 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.30 | 0.55 | â | 76 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 0.28 | 0.11 | 0.35 | 157 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.