Theia 446
0.26
UTI
0.33
CN
0.28
Cdens
0.5
CC3
0.1
Clit
1.0
Cdup
Nm (P>50%)
33
Core radius and density
1.2 [pc], 1.4 [pc-2]
- CN 0.33 Poorly populated
- Cdens 0.28 Loose
- CC3 0.5 Intermediate quality
- Clit 0.1 Rarely studied
- Cdup 1.0 Unique
Overview
Theia 446 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is rarely studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 18.391 | 62.725 | 2.573 | 7.78 | -3.729 | -3.667 |
| Zhang et al. | 2024 | 18.552 | 62.757 | â | â | â | â |
| Cavallo et al. | 2024 | 18.471 | 62.448 | 2.606 | â | â | â |
| Hunt & Reffert | 2023 | 18.552 | 62.757 | 2.6 | 7.731 | -3.698 | -3.616 |
| He et al. | 2022 | 19.13 | 62.233 | 2.612 | 7.862 | -4.104 | â |
| Kounkel & Covey | 2019 | 15.863 | 62.567 | 2.414 | â | â | -1.19 |
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 | 0.39 | 0.725 | 1.15 | 76 | 0.028 | â | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.115(1) | â | â | â |
| Cavallo et al. | 2024 | 0.39 | 1.10 | â | 42 | -0.060 | â | â | â |
| Hunt & Reffert | 2023 | 0.37 | 0.55 | 1.15 | 80 | â | â | â | â |
| He et al. | 2022 | â | 0.90 | â | 71 | â | â | â | â |
| Kounkel & Covey | 2019 | 0.43 | 0.47 | â | 185 | 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 moving group. CMD class: 0.69 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.69 (50th percentile).