NGC 358
Summary
NGC 358 is a poorly populated, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It is poorly studied in the literature.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 16.296 | 62.022 | – | -4.56 | 2.72 | – |
| Loktin & Popova (2017) | 16.29 | 62.022 | – | -0.81 | -3.607 | – |
| Donor et al. (2020) | 16.296 | 62.022 | – | -0.88 | -0.59 | -71.0 |
| UCC | 16.302 | 61.992 | 0.316 | -2.104 | 0.42 | -60.127 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Loktin & Popova (2017) | E(B-V)=0.767, Dist=1052, logt=7.65 |
| Donor et al. (2020) | Fe/H=-0.31 |
Search coordinates in Bayestar19