OCSN 61
0.51
UTI
0.84
CN
1.0
Cdens
1.0
CC3
0.31
Clit
0.74
Cdup
Radius (P>50% members)
37.5 [arcmin]
- CN 0.84 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.31 Poorly studied
- Cdup 0.74 Likely unique
Overview
OCSN 61 is a rich, very dense object of very high C3 quality. Its parallax locates it at a very close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It was recently reported in the literature.
Note: 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. See table with shared members information.
Very close
Low extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 84.063 | -0.592 | 2.558 | -1.029 | -0.633 | 29.898 |
| Zhang et al. | 2024 | 84.084 | -0.402 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.084 | -0.402 | 2.59 | -1.045 | -0.63 | 26.823 |
| Cavallo et al. | 2024 | 84.133 | -0.747 | 2.596 | â | â | â |
| Hunt & Reffert | 2023 | 84.084 | -0.402 | 2.59 | -1.045 | -0.63 | 26.823 |
| Qin et al. | 2023 | 84.14 | -0.45 | 2.57 | -1.08 | -0.62 | 31.65 |
đĄ Note: The UCC values are estimated from its identified members.
| Reference | Year | Dist [kpc] | Av [mag] | DAv [mag] | Age [Myr] | [Fe/H] [dex] | Mass [Msun] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.049* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 100* | â | â |
| Cavallo et al. | 2024 | 0.39 | 0.57 | â | 7 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 0.37 | 0.19 | 0.66 | 12 | â | â | â | â |
| Qin et al. | 2023 | 0.42 | 0.19 | â | 18 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.