HSC 1155
Summary
HSC 1155 is a sparse, very loose object of 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: 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) | 39.984 | 40.556 | 3.488 | -3.867 | -12.664 | -8.058 |
| Cavallo et al. (2024) | 38.711 | 40.437 | 3.508 | – | – | – |
| UCC | 37.401 | 40.629 | 3.493 | -3.729 | -12.464 | -3.717 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=0.161, diffAV50=0.671, MOD50=7.219, logAge50=8.307 |
| Cavallo et al. (2024) | AV50=0.38, dMod50=7.42, logAge50=8.1, [Fe/H]50=0.05 |
Search coordinates in Bayestar19
