FSR 1360
(MWSC 1413)
0.86
UTI
0.62
CN
1.0
Cdens
1.0
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.6 [arcmin]
- CN 0.62 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1360 is a moderately populated, very dense object of very 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, but with a large variance across recent sources for the age, metallicity, and mass 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 | 120.397 | -34.489 | 0.399 | -1.803 | 2.877 | 44.959 |
| Almeida et al. | 2025 | 120.397 | -34.482 | â | â | â | â |
| Hunt & Reffert | 2024 | 120.4 | -34.481 | 0.401 | -1.81 | 2.884 | 33.394 |
| Cavallo et al. | 2024 | 120.404 | -34.475 | 0.404 | â | â | â |
| Hunt & Reffert | 2023 | 120.4 | -34.481 | 0.401 | -1.81 | 2.884 | 33.394 |
| Almeida et al. | 2023 | 120.395 | -34.479 | â | â | â | â |
| Just et al. | 2023 | 120.392 | -34.457 | â | â | â | â |
| Dias et al. | 2021 | 120.397 | -34.482 | 0.382 | -1.807 | 2.834 | â |
| Cantat-Gaudin et al. | 2020 | 120.392 | -34.483 | 0.375 | -1.798 | 2.838 | â |
| Cantat-Gaudin & Anders | 2020 | 120.392 | -34.483 | 0.375 | -1.798 | 2.838 | â |
| Bossini et al. | 2019 | 120.392 | -34.483 | â | â | â | â |
| Bica et al. | 2019 | 120.41 | -34.488 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 120.392 | -34.483 | 0.375 | -1.798 | 2.838 | â |
| Kharchenko et al. | 2016 | 120.392 | -34.457 | â | â | â | â |
| Kharchenko et al. | 2013 | 120.397 | -34.46 | â | -4.62 | 0.86 | â |
| Froebrich et al. | 2007 | 120.412 | -34.49 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 2.12 | 1.34 | â | 157 | â | 287 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 566* | â | â |
| Cavallo et al. | 2024 | 2.56 | 1.49 | â | 141 | 0.370 | â | â | â |
| Hunt & Reffert | 2023 | 2.27 | 1.20 | 1.03 | 246 | â | â | â | â |
| Almeida et al. | 2023 | 2.24 | 1.55 | â | 108 | -0.044 | 409* | 0.50 | â |
| Just et al. | 2023 | â | â | â | 966 | â | 86 | â | â |
| Dias et al. | 2021 | 2.12 | 1.34 | â | 157 | 0.122 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.39 | 1.24 | â | 155 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.48 | â | â | â | â | â | â | â |
| Bossini et al. | 2019 | 2.50 | 1.16 | â | 156 | 0.000 | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.48 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.74 | 0.90 | â | 966 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.74 | 0.90 | â | 966 | 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.
Cavallo et al. (2024)
Gold sample.