Theia 4212
0.04
UTI
0.39
CN
1.0
Cdens
0.5
CC3
0.25
Clit
0.08
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.39 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.25 Poorly studied
- Cdup 0.08 Very likely duplicate
Overview
Theia 4212 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
Relatively 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 | 94.473 | 9.68 | 0.302 | -1.015 | -0.066 | 43.727 |
| Zhang et al. | 2024 | 94.47 | 9.68 | â | â | â | â |
| Hunt & Reffert | 2024 | 94.47 | 9.68 | 0.3 | -0.991 | -0.059 | 43.733 |
| Cavallo et al. | 2024 | 94.532 | 9.697 | 0.302 | â | â | â |
| Hunt & Reffert | 2023 | 94.47 | 9.68 | 0.3 | -0.991 | -0.059 | 43.733 |
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 | -0.326* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 189* | â | â |
| Cavallo et al. | 2024 | 3.16 | 0.90 | â | 427 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.83 | 0.49 | 1.83 | 431 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.