Theia 292
0.23
UTI
0.0
CN
0.54
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
11.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.54 Moderately dense
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 292 is a sparse, moderately dense object of intermediate C3 quality. Its parallax locates it at a 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: 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.
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 | 231.543 | -64.593 | 1.116 | -1.044 | -4.039 | 3.257 |
| Cavallo et al. | 2024 | 228.945 | -65.215 | 1.106 | â | â | â |
| Hunt & Reffert | 2023 | 231.676 | -64.584 | 1.103 | -1.269 | -4.038 | 1.927 |
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 | 0.92 | 0.51 | â | 417 | 0.480 | â | â | â |
| Hunt & Reffert | 2023 | 0.85 | 0.67 | 1.31 | 166 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.