FSR 1209
(MWSC 1105)
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1209 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 106.785 | -13.829 | 0.19 | -0.944 | 0.715 | 77.847 |
| Li et al. | 2025 | 106.785 | -13.827 | 0.19 | -0.928 | 0.689 | â |
| Hunt & Reffert | 2024 | 106.788 | -13.825 | 0.211 | -0.955 | 0.727 | â |
| Cavallo et al. | 2024 | 106.79 | -13.834 | 0.21 | â | â | â |
| Hunt & Reffert | 2023 | 106.788 | -13.825 | 0.211 | -0.955 | 0.727 | â |
| Just et al. | 2023 | 106.761 | -13.818 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 106.785 | -13.827 | 0.19 | -0.928 | 0.689 | â |
| Cantat-Gaudin & Anders | 2020 | 106.785 | -13.827 | 0.19 | -0.928 | 0.689 | â |
| Bica et al. | 2019 | 106.765 | -13.844 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 106.785 | -13.827 | 0.19 | -0.928 | 0.689 | â |
| Kharchenko et al. | 2016 | 106.761 | -13.818 | â | â | â | â |
| Kharchenko et al. | 2013 | 106.767 | -13.82 | â | -0.89 | -2.49 | â |
| Froebrich et al. | 2007 | 106.767 | -13.848 | â | â | â | â |
| Dias et al. | 2002 | 106.767 | -13.848 | â | -0.89 | -2.49 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 5.64 | 1.38 | â | 535 | 0.063 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 716* | â | â |
| Cavallo et al. | 2024 | 3.58 | 1.66 | â | 331 | -0.420 | â | â | â |
| Hunt & Reffert | 2023 | 4.36 | 1.39 | 0.83 | 180 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1318 | â | 1045 | â | â |
| Cantat-Gaudin et al. | 2020 | 5.47 | 1.30 | â | 282 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.58 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.58 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.96 | 1.35 | â | 1318 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.96 | 1.35 | â | 1318 | â | â | â | â |
| Dias et al. | 2002 | 2.96 | 1.35 | â | 1318 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.