FSR 1361
(MWSC 1358; FoF 34)
0.91
UTI
0.87
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
12.9 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1361 is a rich, 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 massive, near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 117.655 | -36.397 | 0.375 | -2.497 | 4.026 | 66.716 |
| Li et al. | 2025 | 117.656 | -36.401 | 0.359 | -2.531 | 4.006 | â |
| Almeida et al. | 2025 | 117.659 | -36.403 | â | â | â | â |
| Hunt & Reffert | 2024 | 117.657 | -36.397 | 0.371 | -2.496 | 4.024 | 66.972 |
| Cavallo et al. | 2024 | 117.66 | -36.403 | 0.377 | â | â | â |
| Hunt & Reffert | 2023 | 117.657 | -36.397 | 0.371 | -2.496 | 4.024 | 66.972 |
| Almeida et al. | 2023 | 117.647 | -36.401 | â | â | â | â |
| Just et al. | 2023 | 117.663 | -36.387 | â | â | â | â |
| Dias et al. | 2021 | 117.659 | -36.403 | 0.366 | -2.536 | 4.004 | 66.225 |
| Cantat-Gaudin et al. | 2020 | 117.656 | -36.401 | 0.359 | -2.531 | 4.006 | â |
| Cantat-Gaudin & Anders | 2020 | 117.656 | -36.401 | 0.359 | -2.531 | 4.006 | â |
| Liu & Pang | 2019 | 117.656 | -36.392 | 0.357 | -2.513 | 3.935 | â |
| Soubiran et al. | 2018 | 117.656 | -36.401 | â | â | â | 66.46 |
| Bica et al. | 2019 | 117.686 | -36.385 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 117.656 | -36.401 | 0.359 | -2.531 | 4.006 | â |
| Kharchenko et al. | 2016 | 117.663 | -36.387 | â | â | â | â |
| Kharchenko et al. | 2013 | 117.667 | -36.39 | â | -1.92 | 6.58 | â |
| Froebrich et al. | 2007 | 117.683 | -36.389 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.425 | 1.99 | 1.82 | 457 | -0.052 | 1138 | 0.61 | â |
| Li et al. | 2025 | 2.43 | 1.77 | â | 758 | 0.069 | â | â | â |
| Almeida et al. | 2025 | 2.08 | 1.94 | â | 615 | â | 1208 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2721(1) | â | â |
| Cavallo et al. | 2024 | 2.42 | 2.22 | â | 457 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 2.44 | 1.99 | 1.82 | 385 | â | â | â | â |
| Almeida et al. | 2023 | 2.19 | 2.05 | â | 550 | -0.093 | 1067(1) | 0.61 | â |
| Just et al. | 2023 | â | â | â | 309 | â | 235 | â | â |
| Dias et al. | 2021 | 2.08 | 1.94 | â | 615 | -0.052 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.72 | 1.73 | â | 288 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.58 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 741 | -1.750 | â | â | â |
| Soubiran et al. | 2018 | 2.58 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.58 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.23 | 2.45 | â | 309 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.23 | 2.45 | â | 309 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: good fit. Isochrone match: intermediate fit.