Theia 3329
0.09
UTI
0.26
CN
0.2
Cdens
0.75
CC3
0.03
Clit
0.35
Cdup
Nm (P>50%)
26
Core radius and density
1.3 [pc], 1.0 [pc-2]
- CN 0.26 Poorly populated
- Cdens 0.2 Very loose
- CC3 0.75 High quality
- Clit 0.03 Rarely studied
- Cdup 0.35 Possibly duplicate
Overview
Theia 3329 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a close distance, above the mid-plane, affected by low 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 possibly a duplicate object, which shares a significant 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 | 255.374 | -25.692 | 1.022 | -0.599 | 0.304 | -18.548 |
| Hunt & Reffert | 2024 | 255.407 | -25.706 | 1.011 | -0.728 | 0.332 | -16.086 |
| Cavallo et al. | 2024 | 255.341 | -25.678 | 1.017 | â | â | â |
| Hunt & Reffert | 2023 | 255.407 | -25.706 | 1.011 | -0.728 | 0.332 | -16.086 |
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 | 0.95 | 0.51 | 0.58 | 291 | 0.210 | 77 | â | â |
| Hunt & Reffert | 2024 | 0.95 | 0.51 | 0.58 | 291 | â | 77(1) | â | â |
| Cavallo et al. | 2024 | 0.99 | 0.84 | â | 115 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 0.95 | 0.51 | 0.58 | 291 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.97 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.97 (50th percentile).