LK 10
(Le Duigou-Knodlseder 10; FSR 0233)
0.66
UTI
0.8
CN
1.0
Cdens
1.0
CC3
0.25
Clit
1.0
Cdup
Stellar density (N50/rad)
52.8 [N/pc2]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
LK 10 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close* distance, near the mid-plane, affected by very high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~1.59 kpc) differs significantly from the median photometric distance (~2.52 kpc).
Note: This object shares a large percentage of members with a later 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 | 99999â | 309.825 | 40.002 | 0.627 | -2.9 | -4.503 | 13.381 |
| Hunt & Reffert | 2024 | 309.835 | 39.996 | 0.613 | -2.921 | -4.5 | 12.654 |
| Cavallo et al. | 2024 | 309.831 | 40.013 | 0.599 | â | â | â |
| Hunt & Reffert | 2023 | 309.835 | 39.996 | 0.613 | -2.921 | -4.5 | 12.654 |
| Bica et al. | 2019 | 309.805 | 39.98 | â | â | â | â |
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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.525 | 6.17 | 2.16 | 330 | 0.550 | 1331 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1331(1) | â | â |
| Cavallo et al. | 2024 | 3.61 | 5.59 | â | 447 | 0.550 | â | â | â |
| Hunt & Reffert | 2023 | 1.44 | 6.75 | 2.16 | 213 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.