OCSN 65
Summary
OCSN 65 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.
This is very likely a unique object, which shares a small percentage of members with at least one previously reported entry, and a small percentage with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Qin et al. (2023) | 83.88 | -1.79 | 2.37 | -1.34 | 0.93 | 26.34 |
| Hunt & Reffert (2023) | 83.764 | -2.155 | 2.365 | -1.258 | 0.93 | 33.161 |
| Cavallo et al. (2024) | 83.749 | -1.836 | 2.362 | – | – | – |
| Hunt & Reffert (2024) | 83.764 | -2.155 | 2.365 | -1.258 | 0.93 | 33.161 |
| UCC | 83.789 | -1.805 | 2.366 | -1.311 | 0.921 | 27.08 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Qin et al. (2023) | E(B-V)=0.19, m-M=8.6, logt=7.15 |
| Hunt & Reffert (2023) | AV50=0.365, diffAV50=0.58, MOD50=8.068, logAge50=7.117 |
| Cavallo et al. (2024) | AV50=0.85, dMod50=8.21, logAge50=6.68, [Fe/H]50=-0.19 |
| Hunt & Reffert (2024) | MassJ=52.2505, MassTot=61.0850 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| Gulliver 6 | 17.6 | 83.34 | -1.63 | 2.41 | -0.07 | -0.24 | 28.06 | 0.68 |
| OCSN 194 | 14.5 | 83.32 | -1.64 | 2.42 | -0.06 | -0.25 | 28.06 | 0.02 |
| OCSN 61 | 0.4 | 84.06 | -0.59 | 2.56 | -1.03 | -0.63 | 29.9 | 0.52 |
