Theia 4912
0.16
UTI
0.0
CN
0.18
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
20.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.18 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 4912 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a close distance, near 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 | 327.127 | 52.594 | 1.204 | -1.814 | -0.823 | -33.436 |
| Cavallo et al. | 2024 | 327.707 | 52.906 | 1.201 | â | â | â |
| Hunt & Reffert | 2023 | 327.098 | 52.548 | 1.196 | -1.8 | -0.772 | -21.245 |
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 | 0.74 | 1.10 | â | 141 | 0.070 | â | â | â |
| Hunt & Reffert | 2023 | 0.81 | 0.89 | 1.38 | 82 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.