Theia 6242
0.04
UTI
0.73
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.06
Cdup
Radius (P>50% members)
3.0 [arcmin]
- CN 0.73 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.06 Very likely duplicate
Overview
Theia 6242 is a moderately populated, very dense object of very high 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, old cluster (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
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 149.03 | -60.18 | 0.334 | -5.875 | 5.223 | 0.659 |
| Hu & Soubiran | 2025 | 149.024 | -60.181 | â | â | â | â |
| Hunt & Reffert | 2024 | 149.006 | -60.184 | 0.332 | -5.878 | 5.212 | 0.265 |
| Cavallo et al. | 2024 | 149.024 | -60.181 | 0.335 | â | â | â |
| Hunt & Reffert | 2023 | 149.006 | -60.184 | 0.332 | -5.878 | 5.212 | 0.265 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.250* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 568* | â | â |
| Cavallo et al. | 2024 | 2.41 | 0.93 | â | 2692 | -0.200 | â | â | â |
| Hunt & Reffert | 2023 | 2.80 | 0.42 | 0.29 | 2193 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.