HSC 2495
Summary
HSC 2495 is a sparse, very loose object of very low C3 quality. It is located at a large 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) | 183.659 | -63.817 | 0.165 | -7.939 | 1.12 | – |
| Hunt & Reffert (2024) | 183.659 | -63.817 | 0.165 | -7.939 | 1.12 | – |
| UCC | 183.67 | -63.815 | 0.164 | -7.944 | 1.119 | -16.504 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.807, diffAV50=2.148, MOD50=13.658, logAge50=8.926 |
| Hunt & Reffert (2024) | MassJ=1385.67, MassTot=1385.67 |
Search coordinates in Bayestar19
