LISC-III 3785
- CN 0.25 Poorly populated
- Cdens 0.17 Very loose
- CC3 0.75 High quality
- Clit 0.0 Rarely studied
- Cdup 0.64 Likely unique
Overview
LISC-III 3785 is a poorly populated, very loose object of high C3 quality. Its parallax locates it at a very close distance, above the mid-plane. It is catalogued as a very metal-poor 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. 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 | – | 270.594 | 22.702 | 3.467 | -1.316 | -7.273 | -18.737 |
| Chi et al. | 2023 | 270.709 | 22.617 | 3.553 | -1.4 | -7.091 | – |
💡 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 |
|---|---|---|---|---|---|---|---|---|---|
| Chi et al. | 2023 | 0.26 | 0.75 | – | – | -1.335 | – | 0.47 | – |
💡 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.
