HSC 2689
Summary
HSC 2689 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well 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) | 254.439 | -69.837 | 0.293 | -3.861 | -7.575 | – |
| Hunt & Reffert (2024) | 254.439 | -69.837 | 0.293 | -3.861 | -7.575 | – |
| UCC | 254.438 | -69.851 | 0.297 | -3.912 | -7.577 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.132, diffAV50=0.921, MOD50=12.295, logAge50=9.869 |
| Hunt & Reffert (2024) | MassJ=72.0960, MassTot=162.251 |
Search coordinates in Bayestar19
