Theia 792
0.62
UTI
0.62
CN
0.98
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
63.4 [arcmin]
- CN 0.62 Moderately populated
- Cdens 0.98 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
Theia 792 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later 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 | 98.93 | 19.625 | 4.706 | 2.906 | -10.782 | 38.732 |
| Zhang et al. | 2024 | 99.018 | 19.613 | â | â | â | â |
| Cavallo et al. | 2024 | 98.625 | 20.494 | 4.752 | â | â | â |
| Hunt & Reffert | 2023 | 99.018 | 19.613 | 4.737 | 3.053 | -11.174 | 38.208 |
| He et al. | 2022 | 99.069 | 19.941 | 4.732 | 2.966 | -10.867 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.077* | â | â | â |
| Cavallo et al. | 2024 | 0.21 | 0.65 | â | 71 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 0.21 | 0.08 | 0.41 | 195 | â | â | â | â |
| He et al. | 2022 | â | 0.25 | â | 100 | 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.