FSR 0306
(FoF 509)
0.71
UTI
0.76
CN
0.58
Cdens
1.0
CC3
0.61
Clit
1.0
Cdup
Nm (P>50%)
120
Core radius and density
2.0 [pc], 2.9 [pc-2]
- CN 0.76 Rich
- Cdens 0.58 Moderately dense
- CC3 1.0 Very high quality
- Clit 0.61 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0306 is a rich, moderately 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 near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Note: This object contains blue stragglers according to at least one source.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 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 |
| Jadhav & Subramaniam | 2021 | 322.129 | 51.69 | â | â | â | â |
| Dias et al. | 2021 | 322.124 | 51.689 | 0.349 | -2.117 | -2.539 | -34.621 |
| Spina et al. | 2021 | 322.13 | 51.696 | 0.355 | -2.11 | -2.56 | â |
| Cantat-Gaudin et al. | 2020 | 322.129 | 51.69 | 0.349 | -2.14 | -2.536 | â |
| Zhong et al. | 2020 | 322.129 | 51.69 | â | -2.14 | -2.536 | -38.787 |
| 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. | 2018 | â | â | â | -3.84 | -4.36 | â |
| Sampedro et al. | 2017 | 322.092 | 51.642 | â | -1.94 | -1.28 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.65 | 3.52 | 2.59 | 258 | 0.150 | 902 | â | 1 |
| Almeida et al. | 2025 | 2.17 | 3.09 | â | 50 | â | 611 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.067(1) | â | â | â |
| Hunt & Reffert | 2024 | 2.59 | 3.85 | 2.59 | 258 | â | 1895(1) | 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 |
| Spina et al. | 2022 | â | â | â | â | 0.155 | â | â | â |
| Jadhav & Subramaniam | 2021 | 2.68 | 2.79 | â | 513 | â | 902 | â | 1(1) |
| Dias et al. | 2021 | 2.17 | 3.09 | â | 50 | 0.180 | â | â | â |
| Spina et al. | 2021 | 2.81 | â | â | 513 | 0.150(20) | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.68 | 2.79 | â | 513 | â | â | â | â |
| Kounkel et al. | 2020 | 2.74 | 3.52 | â | 182 | â | â | â | â |
| Zhong et al. | 2020 | 2.65(1) | â | â | â | 0.000 | 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 | 4.07 | â | 32 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.63 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.63 (50th percentile).
Hu et al. (2021)
Ellipticities (core, all): e_core=0.1401, e_all=0.0493.
Piecka & Paunzen (2021)
Belongs to cluster aggregate 'Agg28' along with NGC 7086.