Theia 4245
0.01
UTI
0.0
CN
0.47
Cdens
0.75
CC3
0.25
Clit
0.04
Cdup
Radius (P>50% members)
12.2 [arcmin]
- CN 0.0 Sparse
- Cdens 0.47 Loose
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.04 Very likely duplicate
Overview
Theia 4245 is a sparse, loose object of high C3 quality. Its parallax locates it at a close 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.
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 | 349.225 | 55.269 | 1.165 | 0.487 | -1.747 | -20.812 |
| Zhang et al. | 2024 | 348.959 | 55.2 | â | â | â | â |
| Hunt & Reffert | 2024 | 348.959 | 55.2 | 1.152 | 0.505 | -1.79 | -21.816 |
| Cavallo et al. | 2024 | 349.207 | 55.194 | 1.152 | â | â | â |
| Hunt & Reffert | 2023 | 348.959 | 55.2 | 1.152 | 0.505 | -1.79 | -21.816 |
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 | 0.104* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 76* | â | â |
| Cavallo et al. | 2024 | 0.88 | 0.67 | â | 219 | 0.660 | â | â | â |
| Hunt & Reffert | 2023 | 0.83 | 0.67 | 0.36 | 109 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.