Theia 2526
0.00
UTI
0.25
CN
0.43
Cdens
0.25
CC3
0.25
Clit
0.0
Cdup
Stellar density (N50/rad)
2.2 [N/pc2]
- CN 0.25 Poorly populated
- Cdens 0.43 Loose
- CC3 0.25 Low quality
- Clit 0.25 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
Theia 2526 is a poorly populated, loose object of low 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, but with a large variance across recent sources for the metallicity parameter (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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 348.12 | 57.481 | 0.907 | 0.267 | -1.365 | -31.891 |
| Zhang et al. | 2024 | 348.108 | 57.485 | â | â | â | â |
| Hunt & Reffert | 2024 | 348.108 | 57.485 | 0.905 | 0.209 | -1.348 | -27.355 |
| Cavallo et al. | 2024 | 347.938 | 57.428 | 0.906 | â | â | â |
| Hunt & Reffert | 2023 | 348.108 | 57.485 | 0.905 | 0.209 | -1.348 | -27.355 |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.135 | 1.675 | 2.11 | 241 | 0.284 | 148 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.101(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 148(1) | â | â |
| Cavallo et al. | 2024 | 1.23 | 1.66 | â | 316 | 0.670 | â | â | â |
| Hunt & Reffert | 2023 | 1.04 | 1.69 | 2.11 | 166 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Part of multiple system G196, along with HSC_890, HSC_854 and HSC_844.
Cavallo et al. (2024)
Gold sample.