Theia 1713
0.02
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.0
Clit
0.04
Cdup
Radius (P>50% members)
8.2 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.04 Very likely duplicate
Overview
Theia 1713 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by moderate 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 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
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 50.222 | 58.927 | 0.915 | 0.509 | -1.612 | -17.567 |
| Hunt & Reffert | 2024 | 50.235 | 58.87 | 0.919 | 0.516 | -1.554 | -20.689 |
| Cavallo et al. | 2024 | 50.162 | 59.031 | 0.917 | â | â | â |
| Hunt & Reffert | 2023 | 50.235 | 58.87 | 0.919 | 0.516 | -1.554 | -20.689 |
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 | 468* | â | â |
| Cavallo et al. | 2024 | 1.16 | 2.41 | â | 4 | -0.180 | â | â | â |
| Hunt & Reffert | 2023 | 1.06 | 2.26 | 1.94 | 4 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.