HSC 675
Summary
HSC 675 is a sparse, very loose object of low C3 quality. It is located at a large distance from the Sun, below the mid-plane. It was recently reported in the literature.This is a unique object, which shares a very small percentage of members with at least one previously reported entry.
Warning: contains less than 25 stars with P>0.5 estimated.
Warning: the low UTI value and no obvious signs of duplication (C_dup=0.96) 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) | 315.711 | 44.764 | 0.107 | -2.596 | -3.344 | -86.906 |
| Cavallo et al. (2024) | 315.743 | 44.753 | 0.107 | – | – | – |
| Hunt & Reffert (2024) | 315.711 | 44.764 | 0.107 | -2.596 | -3.344 | -86.906 |
| UCC | 315.722 | 44.768 | 0.105 | -2.602 | -3.329 | -86.789 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=3.62, diffAV50=2.192, MOD50=14.598, logAge50=8.016 |
| Cavallo et al. (2024) | AV50=1.46, dMod50=14.27, logAge50=8.91, [Fe/H]50=-0.02 |
| Hunt & Reffert (2024) | MassJ=1220.92, MassTot=1263.02 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| FSR 0273 | 4.0 | 315.39 | 44.81 | 0.18 | -2.58 | -3.46 | -59.07 | 0.16 |
