Theia 227
0.01
UTI
0.0
CN
0.36
Cdens
0.75
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members)
24.9 [arcmin]
- CN 0.0 Sparse
- Cdens 0.36 Loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.04 Very likely duplicate
Overview
Theia 227 is a sparse, loose object of high C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young 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.
Very close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 272.02 | -16.619 | 2.08 | 0.008 | -3.873 | -12.302 |
| Cavallo et al. | 2024 | 271.641 | -17.488 | 2.104 | â | â | â |
| Hunt & Reffert | 2023 | 272.09 | -16.473 | 2.108 | 0.019 | -3.979 | -14.445 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.47 | 1.45 | â | 36 | 0.000 | â | â | â |
| Hunt & Reffert | 2023 | 0.46 | 1.35 | 1.90 | 32 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.