FoF 403
(LP 403)
0.70
UTI
0.78
CN
1.0
Cdens
1.0
CC3
0.35
Clit
1.0
Cdup
Stellar density (N50/rad)
26.9 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.35 Poorly studied
- Cdup 1.0 Unique
Overview
FoF 403 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
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 | 161.026 | -58.095 | 0.375 | -7.045 | 2.964 | -11.398 |
| Hunt & Reffert | 2024 | 161.017 | -58.099 | 0.373 | -7.04 | 2.961 | 10.771 |
| Celli et al. | 2024 | 161.024 | -58.095 | â | â | â | â |
| Cavallo et al. | 2024 | 161.042 | -58.097 | 0.374 | â | â | â |
| Hunt & Reffert | 2023 | 161.017 | -58.099 | 0.373 | -7.04 | 2.961 | 10.771 |
| Cantat-Gaudin et al. | 2020 | 161.024 | -58.095 | 0.37 | -7.047 | 2.935 | â |
| Liu & Pang | 2019 | 161.036 | -58.094 | 0.367 | -6.939 | 3.019 | 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 | 2.56 | 1.87 | 2.08 | 26 | 0.430 | 1199 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1420(1) | â | â |
| Celli et al. | 2024 | â | â | â | 26 | â | 978 | â | â |
| Cavallo et al. | 2024 | 2.40 | 1.87 | â | 35 | 0.360 | â | â | â |
| Hunt & Reffert | 2023 | 2.56 | 1.94 | 2.08 | 15 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.77 | 1.35 | â | 26 | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 6 | 0.500 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.