Theia 3975
0.16
UTI
0.0
CN
0.19
Cdens
0.62
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
12.4 [arcmin]
- CN 0.0 Sparse
- Cdens 0.19 Very loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 3975 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young 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.
Relatively close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 122.869 | -42.316 | 0.736 | -5.378 | 4.446 | -21.538 |
| Hunt & Reffert | 2024 | 122.871 | -42.342 | 0.73 | -5.351 | 4.469 | 10.963 |
| Cavallo et al. | 2024 | 122.875 | -42.383 | 0.729 | â | â | â |
| Hunt & Reffert | 2023 | 122.871 | -42.342 | 0.73 | -5.351 | 4.469 | 10.963 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 110* | â | â |
| Cavallo et al. | 2024 | 1.32 | 0.51 | â | 78 | 0.050 | â | â | â |
| Hunt & Reffert | 2023 | 1.30 | 0.49 | 1.12 | 60 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.