FSR 0306
(FoF 509)
0.87
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
3.7 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0306 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
Massive
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 | 322.13 | 51.686 | 0.35 | -2.146 | -2.572 | -37.309 |
| Almeida et al. | 2025 | 322.124 | 51.689 | â | â | â | â |
| Zhang et al. | 2024 | 322.119 | 51.69 | â | â | â | â |
| Hunt & Reffert | 2024 | 322.119 | 51.69 | 0.359 | -2.174 | -2.585 | -28.367 |
| Cavallo et al. | 2024 | 322.125 | 51.693 | 0.358 | â | â | â |
| Hunt & Reffert | 2023 | 322.119 | 51.69 | 0.359 | -2.174 | -2.585 | -28.367 |
| Dias et al. | 2021 | 322.124 | 51.689 | 0.349 | -2.117 | -2.539 | -34.621 |
| Cantat-Gaudin et al. | 2020 | 322.129 | 51.69 | 0.349 | -2.14 | -2.536 | â |
| Cantat-Gaudin & Anders | 2020 | 322.129 | 51.69 | 0.349 | -2.14 | -2.536 | â |
| Liu & Pang | 2019 | 322.133 | 51.678 | 0.335 | -2.099 | -2.558 | â |
| Soubiran et al. | 2018 | 322.129 | 51.69 | â | â | â | -34.63 |
| Cantat-Gaudin et al. | 2018 | 322.129 | 51.69 | 0.349 | -2.14 | -2.536 | â |
| Dias et al. | 2014 | 322.092 | 51.642 | â | -2.46 | -1.66 | â |
| Froebrich et al. | 2007 | 322.092 | 51.642 | â | â | â | â |
| Dias et al. | 2002 | 322.092 | 51.642 | â | -2.46 | -1.66 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.17 | 3.09 | â | 50 | â | 611 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.067* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1895* | â | â |
| Cavallo et al. | 2024 | 2.37 | 3.65 | â | 490 | 0.080 | â | â | â |
| Hunt & Reffert | 2023 | 2.58 | 3.85 | 2.59 | 258 | â | â | â | â |
| Dias et al. | 2021 | 2.17 | 3.09 | â | 50 | 0.180 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.68 | 2.79 | â | 513 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.65 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 871 | 0.500 | â | â | â |
| Soubiran et al. | 2018 | 2.65 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.65 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.33 | 4.00 | â | 32 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.