OCSN 95
- CN 0.72 Moderately populated
- Cdens 0.27 Loose
- CC3 0.62 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 0.94 Very likely unique
Overview
OCSN 95 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a very close distance, near the mid-plane. It is catalogued as a young cluster (see Parameters). It was recently reported in the literature. Note: This is very likely a unique object, which shares a very small percentage of members with at least one previously reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 253.442 | -39.645 | 2.528 | -3.447 | -7.794 | -10.079 |
| Qin et al. | 2023 | 253.45 | -39.49 | 2.57 | -3.47 | -7.89 | -12.76 |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Qin et al. | 2023 | 0.50 | 0.71 | – | 45 | – | – | – | – |
💡 Note: The parameters are sometimes transformed from their original values to match the format of the columns shown here, see FAQ. The columns DAv, Bfr, BSS correspond to differential extinction, binary fraction, and blue stragglers, respectively. BSS values can be listed as fractions or integers.
