OCSN 70
Summary
OCSN 70 is a rich, very dense object of very high 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: This is possibly a duplicated object, which shares a significant percentage of members with at least one previously reported entry.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Qin et al. (2023) | 85.27 | -9.38 | 2.23 | 0.57 | -1.25 | 15.73 |
| Hunt & Reffert (2023) | 85.243 | -9.287 | 2.307 | 0.652 | -1.107 | 17.951 |
| Cavallo et al. (2024) | 85.235 | -9.274 | 2.307 | – | – | – |
| Hunt & Reffert (2024) | 85.243 | -9.287 | 2.307 | 0.652 | -1.107 | 17.951 |
| UCC | 85.34 | -9.446 | 2.272 | 0.529 | -1.214 | 16.144 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Qin et al. (2023) | E(B-V)=0.64, m-M=9.98, logt=6.9 |
| Hunt & Reffert (2023) | AV50=2.969, diffAV50=1.086, MOD50=8.097, logAge50=6.784 |
| Cavallo et al. (2024) | AV50=2.71, dMod50=8.67, logAge50=6.83, [Fe/H]50=0.66 |
| Hunt & Reffert (2024) | MassJ=63.3923, MassTot=63.3923 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OC 0356 | 51.2 | 85.3 | -9.47 | 2.25 | 0.56 | -1.28 | 15.99 | 0.49 |
| FSR 1088 | 15.8 | 85.27 | -9.35 | 2.29 | 0.49 | -1.2 | 16.61 | 0.47 |
| Cmg 109 | 12.0 | 85.25 | -8.97 | 2.22 | 0.48 | -1.0 | 16.48 | 0.45 |
| L 1641S | 1.4 | 85.65 | -8.13 | 2.34 | 0.1 | -0.36 | 15.82 | 0.87 |
