OCSN 56
0.20
UTI
0.7
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.31
Cdup
Radius (P>50% members)
33.1 [arcmin]
- CN 0.7 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.31 Possibly duplicate
Overview
OCSN 56 is a moderately populated, 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.
â ī¸ Warning: This is possibly a duplicate object, which shares a significant percentage of members with at least one previously reported entry, and a significant 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 | 82.645 | 2.366 | 2.526 | -0.816 | 0.526 | 31.28 |
| Zhang et al. | 2024 | 83.578 | 2.629 | â | â | â | â |
| Cavallo et al. | 2024 | 83.432 | 3.614 | 2.389 | â | â | â |
| Hunt & Reffert | 2023 | 83.578 | 2.629 | 2.389 | -0.924 | 0.552 | 25.552 |
| Qin et al. | 2023 | 82.65 | 2.51 | 2.44 | -0.8 | 0.54 | 29.31 |
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 | -0.018* | â | â | â |
| Cavallo et al. | 2024 | 0.43 | 0.80 | â | 7 | -0.220 | â | â | â |
| Hunt & Reffert | 2023 | 0.41 | 0.28 | 0.60 | 11 | â | â | â | â |
| Qin et al. | 2023 | 0.45 | 0.25 | â | 16 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as a moving group.