HSC 905
Summary
HSC 905 is a sparse, moderately dense object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It was recently reported in the literature.
This object shares a large percentage of members with a later 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=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) | 353.438 | 60.04 | 0.225 | -2.086 | -1.235 | -86.107 |
| Hunt & Reffert (2024) | 353.438 | 60.04 | 0.225 | -2.086 | -1.235 | -86.107 |
| UCC | 353.435 | 60.04 | 0.23 | -2.08 | -1.224 | -86.114 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Hunt & Reffert (2023) | AV50=4.493, diffAV50=2.729, MOD50=13.036, logAge50=8.378 |
| Hunt & Reffert (2024) | MassJ=1578.18, MassTot=632.481 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| CWNU 3769 | 80.0 | 353.44 | 60.04 | 0.23 | -2.12 | -1.23 | -86.11 | 0.06 |
