HSC 338
Summary
HSC 338 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, near the mid-plane. It was recently reported in the literature.
Warning: contains less than 25 stars with P>0.5 estimated.
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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 283.636 | 2.902 | 0.429 | -0.637 | -2.685 | 49.026 |
| Cavallo et al. (2024) | 283.74 | 2.884 | 0.449 | – | – | – |
| Hunt & Reffert (2024) | 283.636 | 2.902 | 0.429 | -0.637 | -2.685 | 49.026 |
| UCC | 283.633 | 2.875 | 0.406 | -0.6 | -2.662 | -45.505 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=4.372, diffAV50=3.124, MOD50=11.374, logAge50=8.076 |
| Cavallo et al. (2024) | AV50=4.86, dMod50=12.29, logAge50=7.58, [Fe/H]50=0.72 |
| Hunt & Reffert (2024) | MassJ=4534.92, MassTot=8888.75 |
Search coordinates in Bayestar19