FSR 0324
(MWSC 3533)
0.55
UTI
0.36
CN
0.54
Cdens
0.75
CC3
0.55
Clit
1.0
Cdup
Stellar density (N50/rad)
2.7 [N/pc2]
- CN 0.36 Poorly populated
- Cdens 0.54 Moderately dense
- CC3 0.75 High quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0324 is a poorly populated, moderately dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 324.055 | 53.843 | 0.287 | -2.794 | -2.974 | â |
| Hunt & Reffert | 2024 | 324.053 | 53.856 | 0.287 | -2.786 | -2.963 | â |
| Cavallo et al. | 2024 | 324.036 | 53.834 | 0.285 | â | â | â |
| Hunt & Reffert | 2023 | 324.053 | 53.856 | 0.287 | -2.786 | -2.963 | â |
| Just et al. | 2023 | 324.04 | 53.801 | â | â | â | â |
| Kharchenko et al. | 2016 | 324.04 | 53.801 | â | â | â | â |
| Dias et al. | 2014 | 324.038 | 53.815 | â | -4.24 | -1.34 | â |
| Kharchenko et al. | 2013 | 324.045 | 53.805 | â | -4.25 | -2.37 | â |
| Kharchenko et al. | 2012 | 324.045 | 53.805 | â | -3.21 | -2.43 | â |
| Froebrich et al. | 2007 | 324.038 | 53.815 | â | â | â | â |
| Dias et al. | 2002 | 324.038 | 53.815 | â | -4.24 | -1.34 | 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 | 4.17 | 2.705 | 0.45 | 151 | 0.200 | 378 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 398(1) | â | â |
| Cavallo et al. | 2024 | 3.31 | 2.83 | â | 51 | 0.200 | â | â | â |
| Hunt & Reffert | 2023 | 3.40 | 2.58 | 0.45 | 54 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 151 | â | 357 | â | â |
| Kharchenko et al. | 2016 | 4.17 | 2.90 | â | 151 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.17 | 2.90 | â | 151 | â | â | â | â |
| Kharchenko et al. | 2012 | 4.50 | 2.05 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 4.50 | 2.05 | â | 1000 | 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)
Gold sample.