FSR 0241
(MWSC 3236)
0.88
UTI
0.75
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
5.2 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0241 is a rich, very dense object of very 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, old cluster (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 300.782 | 46.195 | 0.451 | -1.413 | -3.582 | 12.206 |
| Li et al. | 2025 | 300.763 | 46.196 | 0.45 | -1.427 | -3.575 | â |
| Hu & Soubiran | 2025 | 300.751 | 46.192 | â | â | â | â |
| Almeida et al. | 2025 | 300.749 | 46.195 | â | â | â | â |
| Zhang et al. | 2024 | 300.76 | 46.195 | â | â | â | â |
| Hunt & Reffert | 2024 | 300.76 | 46.195 | 0.444 | -1.411 | -3.574 | 10.722 |
| Cavallo et al. | 2024 | 300.751 | 46.192 | 0.449 | â | â | â |
| Hunt & Reffert | 2023 | 300.76 | 46.195 | 0.444 | -1.411 | -3.574 | 10.722 |
| Almeida et al. | 2023 | 300.758 | 46.181 | â | â | â | â |
| Dias et al. | 2021 | 300.749 | 46.195 | 0.459 | -1.403 | -3.611 | -1.102 |
| Cantat-Gaudin et al. | 2020 | 300.763 | 46.196 | 0.45 | -1.427 | -3.575 | â |
| Cantat-Gaudin & Anders | 2020 | 300.763 | 46.196 | 0.45 | -1.427 | -3.575 | â |
| Soubiran et al. | 2018 | 300.763 | 46.196 | â | â | â | -0.52 |
| Bica et al. | 2019 | 300.761 | 46.192 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 300.763 | 46.196 | 0.45 | -1.427 | -3.575 | â |
| Froebrich et al. | 2007 | 300.758 | 46.189 | 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 | 2.08 | 1.09 | â | 1203 | 0.051 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.090* | â | â | â |
| Almeida et al. | 2025 | 2.08 | 1.33 | â | 1205 | â | 293 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.034* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 594* | â | â |
| Cavallo et al. | 2024 | 2.11 | 1.30 | â | 955 | 0.210 | â | â | â |
| Hunt & Reffert | 2023 | 2.11 | 1.04 | 0.60 | 1178 | â | â | â | â |
| Almeida et al. | 2023 | 2.06 | 1.32 | â | 1202 | -0.031 | 551* | 0.58 | â |
| Dias et al. | 2021 | 2.08 | 1.33 | â | 1205 | -0.045 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.02 | 1.03 | â | 1318 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.09 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.09 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.09 | â | â | â | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.