Theia 3428
0.00
UTI
0.43
CN
1.0
Cdens
0.75
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members)
5.9 [arcmin]
- CN 0.43 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.25 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 3428 is a poorly populated, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below 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 | 90.319 | 4.565 | 0.717 | 0.479 | -2.076 | 33.6 |
| Zhang et al. | 2024 | 90.301 | 4.602 | â | â | â | â |
| Hunt & Reffert | 2024 | 90.301 | 4.602 | 0.707 | 0.465 | -2.07 | 48.074 |
| Cavallo et al. | 2024 | 90.338 | 4.527 | 0.712 | â | â | â |
| Hunt & Reffert | 2023 | 90.301 | 4.602 | 0.707 | 0.465 | -2.07 | 48.074 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.001* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 343* | â | â |
| Cavallo et al. | 2024 | 1.43 | 2.00 | â | 282 | 0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.31 | 1.87 | 2.52 | 141 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.