FSR 0823
(MWSC 650)
0.31
UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.8 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0823 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~2.81 kpc) differs significantly from the median photometric distance (~1.10 kpc).
Note: This object shares a moderate 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 | 85.654 | 29.559 | 0.355 | 1.083 | -1.238 | -14.703 |
| Just et al. | 2023 | 85.637 | 29.549 | â | â | â | â |
| Donor et al. | 2020 | 85.645 | 29.548 | â | 1.3 | -2.07 | 5.4 |
| Bica et al. | 2019 | 85.662 | 29.571 | â | â | â | â |
| Kharchenko et al. | 2016 | 85.637 | 29.549 | â | â | â | â |
| Kharchenko et al. | 2013 | 85.645 | 29.548 | â | 4.01 | -2.45 | â |
| Kharchenko et al. | 2012 | 85.645 | 29.548 | â | 4.01 | -2.45 | â |
| Froebrich et al. | 2007 | 85.658 | 29.566 | â | â | â | â |
| Dias et al. | 2002 | 85.658 | 29.566 | â | 1.44 | -4.71 | 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 | 1.1 | 1.71 | â | 638 | -0.200 | 20 | â | â |
| Just et al. | 2023 | â | â | â | 638 | â | 20 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.200 | â | â | â |
| Kharchenko et al. | 2016 | 1.10 | 1.71 | â | 638 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.10 | 1.71 | â | 638 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.10 | 1.71 | â | 638 | â | â | â | â |
| Dias et al. | 2002 | 1.10 | 1.71 | â | 638 | â | â | â | â |
MOCA
