Theia 35
0.30
UTI
0.27
CN
0.72
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
22.4 [arcmin]
- CN 0.27 Poorly populated
- Cdens 0.72 Moderately dense
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 35 is a poorly populated, moderately dense object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Very close
Low 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 | 107.92 | -19.376 | 2.374 | -7.998 | 3.71 | 24.938 |
| Cavallo et al. | 2024 | 107.933 | -19.602 | 2.394 | â | â | â |
| Hunt & Reffert | 2023 | 107.597 | -19.414 | 2.377 | -8.062 | 3.702 | 22.118 |
| He et al. | 2022 | 108.031 | -19.328 | 2.403 | -8.093 | 3.683 | â |
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 | 0.44 | 0.65 | â | 25 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 0.40 | 0.14 | 0.71 | 30 | â | â | â | â |
| He et al. | 2022 | â | 0.45 | â | 35 | â | â | â | â |
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.