HSC 1987
Summary
HSC 1987 is a sparse, very loose object of intermediate C3 quality. It is located at a relatively close distance from the Sun, above 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) | 123.881 | -27.631 | 0.735 | -4.896 | 4.328 | 47.68 |
| Cavallo et al. (2024) | 123.346 | -27.442 | 0.737 | – | – | – |
| UCC | 123.885 | -27.62 | 0.722 | -4.902 | 4.381 | 29.187 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.479, diffAV50=0.71, MOD50=10.546, logAge50=7.718 |
| Cavallo et al. (2024) | AV50=0.62, dMod50=10.29, logAge50=7.57, [Fe/H]50=-0.37 |
Search coordinates in Bayestar19
