FSR 0905
(MWSC 904; FoF 1974)
0.91
UTI
0.78
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
7.7 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0905 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is very well-studied in the literature.
Relatively close
Low 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 | 98.426 | 22.328 | 0.647 | 1.861 | -3.814 | 3.39 |
| Li et al. | 2025 | 98.442 | 22.312 | 0.649 | 1.965 | -3.85 | â |
| Hu & Soubiran | 2025 | 98.43 | 22.334 | â | â | â | â |
| Almeida et al. | 2025 | 98.438 | 22.31 | â | â | â | â |
| Zhang et al. | 2024 | 98.431 | 22.313 | â | â | â | â |
| Hunt & Reffert | 2024 | 98.431 | 22.313 | 0.644 | 1.851 | -3.805 | 2.159 |
| Cavallo et al. | 2024 | 98.431 | 22.334 | 0.643 | â | â | â |
| Hunt & Reffert | 2023 | 98.431 | 22.313 | 0.644 | 1.851 | -3.805 | 2.159 |
| Almeida et al. | 2023 | 98.429 | 22.325 | â | â | â | â |
| Just et al. | 2023 | 98.418 | 22.289 | â | â | â | â |
| Tarricq et al. | 2022 | 98.454 | 22.333 | 0.644 | 1.836 | -3.819 | â |
| Dias et al. | 2021 | 98.438 | 22.31 | 0.647 | 1.961 | -3.849 | â |
| Cantat-Gaudin et al. | 2020 | 98.442 | 22.312 | 0.649 | 1.965 | -3.85 | â |
| Cantat-Gaudin & Anders | 2020 | 98.442 | 22.312 | 0.649 | 1.965 | -3.85 | â |
| Liu & Pang | 2019 | 98.425 | 22.341 | 0.637 | 1.887 | -3.839 | â |
| Bica et al. | 2019 | 98.442 | 22.295 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 98.442 | 22.312 | 0.649 | 1.965 | -3.85 | â |
| Kharchenko et al. | 2016 | 98.418 | 22.289 | â | â | â | â |
| Kharchenko et al. | 2013 | 98.427 | 22.288 | â | 0.35 | -4.59 | â |
| Froebrich et al. | 2007 | 98.433 | 22.294 | â | â | â | 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 | 1.42 | 0.42 | â | 752 | -0.146 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.150* | â | â | â |
| Almeida et al. | 2025 | 1.42 | 0.48 | â | 643 | â | 112 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.171* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 396* | â | â |
| Cavallo et al. | 2024 | 1.24 | 0.63 | â | 871 | -0.490 | â | â | â |
| Hunt & Reffert | 2023 | 1.45 | 0.21 | 0.98 | 773 | â | â | â | â |
| Almeida et al. | 2023 | 1.41 | 0.53 | â | 600 | -0.086 | 145* | 0.52 | â |
| Just et al. | 2023 | â | â | â | 200 | â | 194 | â | â |
| Tarricq et al. | 2022 | 1.38 | â | â | 417 | â | â | â | â |
| Dias et al. | 2021 | 1.42 | 0.48 | â | 643 | -0.077 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.43 | 0.50 | â | 389 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.48 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 355 | 0.250 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.48 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.79 | 1.16 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.79 | 1.16 | â | 200 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.