OC 0395
0.00
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.25
Clit
0.0
Cdup
Radius (P>50% members)
18.2 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 0.0 Very likely duplicate
Overview
OC 0395 is a rich, very dense object of very high C3 quality. Its parallax locates it at a close distance, below the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: This is very likely a duplicate object, which shares a large percentage of members with at least one previously reported entry. See table with shared members information.
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 | 104.352 | -21.284 | 1.211 | -3.49 | 3.257 | 36.283 |
| Hunt & Reffert | 2024 | 104.369 | -21.353 | 1.222 | -3.468 | 3.255 | 34.798 |
| Cavallo et al. | 2024 | 104.294 | -21.338 | 1.216 | â | â | â |
| Hunt & Reffert | 2023 | 104.369 | -21.353 | 1.222 | -3.468 | 3.255 | 34.798 |
| Hao et al. | 2022 | 104.291 | -21.273 | 1.195 | -3.486 | 3.286 | 72.312 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 189* | â | â |
| Cavallo et al. | 2024 | 0.84 | 0.39 | â | 11 | -0.190 | â | â | â |
| Hunt & Reffert | 2023 | 0.79 | 0.16 | 0.52 | 15 | â | â | â | â |
| Hao et al. | 2022 | â | 0.67 | â | 20 | 0.611 | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.
Cavallo et al. (2024)
Gold sample.