FSR 1399
(MWSC 1546)
0.80
UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.4 [arcmin]
- CN 0.58 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1399 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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 metallicity parameter (see Parameters). It is well-studied in the literature.
Relatively close
High 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 | 131.034 | -39.352 | 0.333 | -4.06 | 3.446 | 94.26 |
| Hu & Soubiran | 2025 | 131.042 | -39.351 | â | â | â | â |
| Almeida et al. | 2025 | 131.037 | -39.351 | â | â | â | â |
| Hunt & Reffert | 2024 | 131.04 | -39.355 | 0.324 | -4.032 | 3.446 | 89.413 |
| Cavallo et al. | 2024 | 131.042 | -39.351 | 0.329 | â | â | â |
| Hunt & Reffert | 2023 | 131.04 | -39.355 | 0.324 | -4.032 | 3.446 | 89.413 |
| Almeida et al. | 2023 | 131.039 | -39.349 | â | â | â | â |
| Just et al. | 2023 | 131.035 | -39.362 | â | â | â | â |
| Dias et al. | 2021 | 131.037 | -39.351 | 0.314 | -4.123 | 3.372 | â |
| Cantat-Gaudin et al. | 2020 | 131.035 | -39.352 | 0.315 | -4.111 | 3.387 | â |
| Cantat-Gaudin & Anders | 2020 | 131.035 | -39.352 | 0.315 | -4.111 | 3.387 | â |
| Bica et al. | 2019 | 131.062 | -39.366 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 131.035 | -39.352 | 0.315 | -4.111 | 3.387 | â |
| Kharchenko et al. | 2016 | 131.035 | -39.362 | â | â | â | â |
| Kharchenko et al. | 2013 | 131.04 | -39.365 | â | -4.38 | 8.07 | â |
| Froebrich et al. | 2007 | 131.058 | -39.37 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | 0.000* | â | â | â |
| Almeida et al. | 2025 | 2.78 | 3.03 | â | 625 | â | 366 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 621* | â | â |
| Cavallo et al. | 2024 | 2.77 | 3.12 | â | 631 | 0.500 | â | â | â |
| Hunt & Reffert | 2023 | 2.66 | 2.69 | 2.25 | 233 | â | â | â | â |
| Almeida et al. | 2023 | 2.56 | 3.12 | â | 590 | -0.017 | 351* | 0.62 | â |
| Just et al. | 2023 | â | â | â | 200 | â | 843 | â | â |
| Dias et al. | 2021 | 2.78 | 3.03 | â | 625 | 0.020 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.92 | 2.70 | â | 977 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.90 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.90 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.31 | 3.87 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.31 | 3.87 | 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: intermediate fit. Silver sample.
Cavallo et al. (2024)
Gold sample.