Theia 3475
0.12
UTI
0.33
CN
0.27
Cdens
0.38
CC3
0.25
Clit
0.39
Cdup
Stellar density (N50/rad)
1.3 [N/pc2]
- CN 0.33 Poorly populated
- Cdens 0.27 Loose
- CC3 0.38 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.39 Possibly duplicate
Overview
Theia 3475 is a poorly populated, loose object of low C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 93.252 | 24.106 | 0.521 | 0.145 | -1.969 | 664.495 |
| Zhang et al. | 2024 | 93.198 | 24.112 | â | â | â | â |
| Hunt & Reffert | 2024 | 93.198 | 24.112 | 0.516 | 0.146 | -1.996 | 664.493 |
| Cavallo et al. | 2024 | 93.21 | 23.9 | 0.516 | â | â | â |
| Hunt & Reffert | 2023 | 93.198 | 24.112 | 0.516 | 0.146 | -1.996 | 664.493 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.85 | 1.525 | 2.38 | 164 | -0.267 | 242 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.193(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 242(1) | â | â |
| Cavallo et al. | 2024 | 1.86 | 1.56 | â | 182 | -0.340 | â | â | â |
| Hunt & Reffert | 2023 | 1.84 | 1.49 | 2.38 | 145 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.