HSC 1730
Summary
HSC 1730 is a poorly populated, very loose object of very low C3 quality. It is located at a very close distance from the Sun, below the mid-plane. It was recently reported 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 |
|---|---|---|---|---|---|---|
| Hunt & Reffert (2023) | 32.913 | -27.551 | 2.215 | 30.043 | -15.034 | 39.913 |
| UCC | 32.347 | -27.553 | 2.255 | 29.855 | -15.304 | 25.905 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.143, diffAV50=0.331, MOD50=8.213, logAge50=9.473 |
Search coordinates in Bayestar19
