FSR 0728
(MWSC 384)
0.80
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0728 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, below the mid-plane, affected by moderate 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 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 | 67.458 | 38.493 | 0.558 | 1.916 | -2.269 | 19.97 |
| Li et al. | 2025 | 67.458 | 38.496 | 0.543 | 1.991 | -2.224 | â |
| Almeida et al. | 2025 | 67.459 | 38.492 | â | â | â | â |
| Zhang et al. | 2024 | 67.462 | 38.498 | â | â | â | â |
| Hunt & Reffert | 2024 | 67.462 | 38.498 | 0.548 | 1.92 | -2.273 | 24.889 |
| Cavallo et al. | 2024 | 67.45 | 38.476 | 0.55 | â | â | â |
| Hunt & Reffert | 2023 | 67.462 | 38.498 | 0.548 | 1.92 | -2.273 | 24.889 |
| Almeida et al. | 2023 | 67.468 | 38.489 | â | â | â | â |
| Dias et al. | 2021 | 67.459 | 38.492 | 0.533 | 1.968 | -2.237 | â |
| Cantat-Gaudin et al. | 2020 | 67.458 | 38.496 | 0.543 | 1.991 | -2.224 | â |
| Cantat-Gaudin & Anders | 2020 | 67.458 | 38.496 | 0.543 | 1.991 | -2.224 | â |
| Bica et al. | 2019 | 67.456 | 38.488 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 67.458 | 38.496 | 0.543 | 1.991 | -2.224 | â |
| Froebrich et al. | 2007 | 67.454 | 38.485 | 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 | 1.57 | 1.98 | â | 399 | 0.007 | â | â | â |
| Almeida et al. | 2025 | 1.58 | 2.29 | â | 136 | â | 325 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.193* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 646* | â | â |
| Cavallo et al. | 2024 | 1.76 | 2.15 | â | 257 | 0.270 | â | â | â |
| Hunt & Reffert | 2023 | 1.70 | 1.95 | 2.50 | 385 | â | â | â | â |
| Almeida et al. | 2023 | 1.53 | 2.14 | â | 115 | -0.040 | 321* | 0.63 | â |
| Dias et al. | 2021 | 1.58 | 2.29 | â | 136 | -0.087 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.88 | 1.76 | â | 162 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.75 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.75 | 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: good fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.