Theia 560
0.04
UTI
0.28
CN
0.12
Cdens
0.12
CC3
0.0
Clit
0.36
Cdup
Radius (P>50% members)
34.7 [arcmin]
- CN 0.28 Poorly populated
- Cdens 0.12 Very loose
- CC3 0.12 Very low quality
- Clit 0.0 Rarely studied
- Cdup 0.36 Possibly duplicate
Overview
Theia 560 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a close distance, near 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 possibly a duplicate object, which shares a significant 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 | 73.665 | 45.926 | 1.493 | -1.293 | -2.968 | -7.69 |
| Zhang et al. | 2024 | 73.595 | 45.869 | â | â | â | â |
| Cavallo et al. | 2024 | 73.479 | 46.254 | 1.509 | â | â | â |
| Hunt & Reffert | 2023 | 73.595 | 45.869 | 1.51 | -1.283 | -2.93 | -8.822 |
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 | -0.144* | â | â | â |
| Cavallo et al. | 2024 | 0.68 | 0.82 | â | 407 | 0.530 | â | â | â |
| Hunt & Reffert | 2023 | 0.62 | 0.78 | 0.74 | 212 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.