HSC 2618
Summary
HSC 2618 is a sparse, very loose object of low C3 quality. It is located at a very close 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) | 210.971 | -65.803 | 5.056 | -16.808 | -10.07 | 9.442 |
| Cavallo et al. (2024) | 211.751 | -65.928 | 5.066 | – | – | – |
| UCC | 214.971 | -65.423 | 4.994 | -16.571 | -10.043 | 8.29 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.374, diffAV50=0.773, MOD50=6.505, logAge50=7.339 |
| Cavallo et al. (2024) | AV50=1.0, dMod50=6.37, logAge50=7.19, [Fe/H]50=-0.26 |
Search coordinates in Bayestar19
