HSC 2693
Summary
HSC 2693 is a sparse, very loose object of high C3 quality. It is located at a relatively close distance from the Sun, below 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) | 239.473 | -63.826 | 0.67 | -2.197 | -5.65 | -51.898 |
| Cavallo et al. (2024) | 239.756 | -63.813 | 0.669 | – | – | – |
| UCC | 239.573 | -63.816 | 0.674 | -2.206 | -5.656 | -38.934 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.221, diffAV50=0.308, MOD50=10.743, logAge50=8.796 |
| Cavallo et al. (2024) | AV50=0.3, dMod50=10.66, logAge50=8.68, [Fe/H]50=0.44 |
Search coordinates in Bayestar19
