LISC-III 3682
0.28
UTI
0.6
CN
0.27
Cdens
0.5
CC3
0.0
Clit
1.0
Cdup
Radius (P>50% members)
42.3 [arcmin]
- CN 0.6 Moderately populated
- Cdens 0.27 Loose
- CC3 0.5 Intermediate quality
- Clit 0.0 Rarely studied
- Cdup 1.0 Unique
Overview
LISC-III 3682 is a moderately populated, loose object of intermediate C3 quality. Its parallax locates it at a close distance, near the mid-plane. It is catalogued as a near-solar metallicity cluster (see Parameters). It was recently reported in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | – | 106.584 | -22.369 | 1.698 | -4.499 | 3.155 | 29.547 |
| Chi et al. | 2023 | 106.968 | -22.362 | 1.826 | -4.547 | 2.989 | – |
💡 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 | 0.66 | 0.60 | – | – | -0.419 | – | 0.45 | – |
💡 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.
