OCSN 61
Summary
OCSN 61 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 likely a unique object, which shares a moderate percentage of members with at least one previously reported entry, and a moderate percentage with at least one entry reported in the same catalogue.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Qin et al. (2023) | 84.14 | -0.45 | 2.57 | -1.08 | -0.62 | 31.65 |
| Hunt & Reffert (2023) | 84.084 | -0.402 | 2.59 | -1.045 | -0.63 | 26.823 |
| Cavallo et al. (2024) | 84.133 | -0.747 | 2.596 | – | – | – |
| Hunt & Reffert (2024) | 84.084 | -0.402 | 2.59 | -1.045 | -0.63 | 26.823 |
| UCC | 84.063 | -0.592 | 2.558 | -1.029 | -0.633 | 29.898 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Qin et al. (2023) | E(B-V)=0.06, m-M=8.12, logt=7.25 |
| Hunt & Reffert (2023) | AV50=0.19, diffAV50=0.655, MOD50=7.855, logAge50=7.069 |
| Cavallo et al. (2024) | AV50=0.57, dMod50=7.96, logAge50=6.87, [Fe/H]50=-0.13 |
| Hunt & Reffert (2024) | MassJ=99.7738, MassTot=111.773 |
Search coordinates in Bayestar19
Cluster region map
Objects with shared members
| Cluster | % | RA | DEC | Plx | pmRA | pmDE | Rv | UTI |
|---|---|---|---|---|---|---|---|---|
| OCSN 194 | 27.1 | 83.32 | -1.64 | 2.42 | -0.06 | -0.25 | 28.06 | 0.02 |
| Gulliver 6 | 26.2 | 83.34 | -1.63 | 2.41 | -0.07 | -0.24 | 28.06 | 0.68 |
| OC 0340 | 5.0 | 84.54 | -0.18 | 2.44 | -0.07 | -0.62 | 24.57 | 0.45 |
| OCSN 65 | 0.3 | 83.79 | -1.81 | 2.37 | -1.31 | 0.92 | 27.08 | 0.57 |
| OCSN 66 | 0.3 | 85.38 | -1.87 | 2.5 | 0.07 | -0.89 | 24.93 | 0.44 |
