HSC 2489
Summary
HSC 2489 is a sparse, very loose object of low 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) | 180.846 | -67.385 | 0.6 | -5.822 | 0.94 | – |
| Hunt & Reffert (2024) | 180.846 | -67.385 | 0.6 | -5.822 | 0.94 | – |
| UCC | 180.864 | -67.374 | 0.569 | -5.842 | 0.946 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=1.437, diffAV50=0.827, MOD50=11.1, logAge50=9.919 |
| Hunt & Reffert (2024) | MassJ=68.5751, MassTot=116.327 |
Search coordinates in Bayestar19
