Theia 1777
0.00
UTI
0.7
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.0
Cdup
Radius (P>50% members)
3.2 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 1777 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age 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.
Relatively close
Moderate 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 | 258.815 | -36.571 | 0.634 | -1.034 | 0.524 | -31.289 |
| Hunt & Reffert | 2024 | 258.814 | -36.575 | 0.634 | -1.044 | 0.504 | -24.044 |
| Cavallo et al. | 2024 | 258.821 | -36.571 | 0.63 | â | â | â |
| Hunt & Reffert | 2023 | 258.814 | -36.575 | 0.634 | -1.044 | 0.504 | -24.044 |
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 | 422* | â | â |
| Cavallo et al. | 2024 | 1.49 | 2.40 | â | 158 | 0.150 | â | â | â |
| Hunt & Reffert | 2023 | 1.48 | 2.32 | 1.17 | 148 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.