Theia 1934
0.09
UTI
0.41
CN
0.79
Cdens
0.75
CC3
0.0
Clit
0.22
Cdup
Radius (P>50% members)
9.4 [arcmin]
- CN 0.41 Poorly populated
- Cdens 0.79 Dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.22 Likely duplicate
Overview
Theia 1934 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
â ī¸ Warning: This is 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
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 196.383 | -56.883 | 0.846 | -6.254 | -0.812 | -2.711 |
| Hunt & Reffert | 2024 | 196.386 | -56.855 | 0.846 | -6.281 | -0.845 | -3.617 |
| Cavallo et al. | 2024 | 196.252 | -57.134 | 0.849 | â | â | â |
| Hunt & Reffert | 2023 | 196.386 | -56.855 | 0.846 | -6.281 | -0.845 | -3.617 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 272* | â | â |
| Cavallo et al. | 2024 | 1.15 | 0.86 | â | 9 | -0.310 | â | â | â |
| Hunt & Reffert | 2023 | 1.14 | 0.75 | 1.25 | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.