FSR 0735
(MWSC 433)
0.82
UTI
0.61
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
2.6 [arcmin]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0735 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Relatively close
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 | 73.468 | 40.858 | 0.311 | 0.419 | -2.109 | â |
| Li et al. | 2025 | 73.471 | 40.859 | 0.316 | 0.512 | -2.068 | â |
| Almeida et al. | 2025 | 73.488 | 40.865 | â | â | â | â |
| Hunt & Reffert | 2024 | 73.471 | 40.858 | 0.312 | 0.408 | -2.103 | â |
| Cavallo et al. | 2024 | 73.47 | 40.862 | 0.315 | â | â | â |
| Hunt & Reffert | 2023 | 73.471 | 40.858 | 0.312 | 0.408 | -2.103 | â |
| Almeida et al. | 2023 | 73.482 | 40.862 | â | â | â | â |
| Dias et al. | 2021 | 73.488 | 40.865 | 0.323 | 0.56 | -2.06 | â |
| Cantat-Gaudin et al. | 2020 | 73.471 | 40.859 | 0.316 | 0.512 | -2.068 | â |
| Cantat-Gaudin & Anders | 2020 | 73.471 | 40.859 | 0.316 | 0.512 | -2.068 | â |
| Bossini et al. | 2019 | 73.471 | 40.859 | â | â | â | â |
| Soubiran et al. | 2018 | 73.471 | 40.859 | â | â | â | 23.62 |
| Bica et al. | 2019 | 73.49 | 40.833 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 73.471 | 40.859 | 0.316 | 0.512 | -2.068 | â |
| Dias et al. | 2014 | 73.471 | 40.862 | â | -0.13 | -1.66 | â |
| Froebrich et al. | 2007 | 73.487 | 40.834 | â | â | â | â |
| Dias et al. | 2002 | 73.471 | 40.862 | â | -0.13 | -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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.71 | 1.59 | â | 508 | -0.144 | â | â | â |
| Almeida et al. | 2025 | 2.58 | 1.63 | â | 514 | â | 356 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 574* | â | â |
| Cavallo et al. | 2024 | 2.65 | 1.69 | â | 309 | -0.100 | â | â | â |
| Hunt & Reffert | 2023 | 2.89 | 1.53 | 0.59 | 171 | â | â | â | â |
| Almeida et al. | 2023 | 2.57 | 1.64 | â | 468 | -0.175 | 392* | 0.59 | â |
| Dias et al. | 2021 | 2.58 | 1.63 | â | 514 | -0.135 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.86 | 1.13 | â | 457 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.90 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 3.35 | 1.43 | â | 279 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 2.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.90 | â | â | â | â | â | â | â |
| Dias et al. | 2002 | 2.50 | 1.58 | â | 501 | 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.
Cavallo et al. (2024)
Gold sample.