FSR 1113
(MWSC 1126)
0.80
UTI
0.52
CN
1.0
Cdens
0.75
CC3
0.87
Clit
1.0
Cdup
Stellar density (N50/rad)
7.1 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.87 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1113 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 low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the age and mass parameters (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 | 107.3 | -1.505 | 0.209 | -0.567 | 1.907 | 71.761 |
| Li et al. | 2025 | 107.3 | -1.502 | 0.254 | -0.566 | 1.913 | â |
| Hu & Soubiran | 2025 | 107.309 | -1.487 | â | â | â | â |
| Almeida et al. | 2025 | 107.302 | -1.507 | â | â | â | â |
| Hunt & Reffert | 2024 | 107.295 | -1.505 | 0.208 | -0.55 | 1.894 | 72.24 |
| Cavallo et al. | 2024 | 107.309 | -1.487 | 0.209 | â | â | â |
| Hunt & Reffert | 2023 | 107.295 | -1.505 | 0.208 | -0.55 | 1.894 | 72.24 |
| Just et al. | 2023 | 107.281 | -1.498 | â | â | â | â |
| Dias et al. | 2021 | 107.302 | -1.507 | 0.271 | -0.555 | 1.884 | â |
| Cantat-Gaudin et al. | 2020 | 107.3 | -1.502 | 0.254 | -0.566 | 1.913 | â |
| Donor et al. | 2020 | 107.287 | -1.5 | â | -0.46 | 1.84 | 69.0 |
| Cantat-Gaudin & Anders | 2020 | 107.3 | -1.502 | 0.254 | -0.566 | 1.913 | â |
| Bica et al. | 2019 | 107.289 | -1.51 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 107.3 | -1.502 | 0.254 | -0.566 | 1.913 | â |
| Kharchenko et al. | 2016 | 107.281 | -1.498 | â | â | â | â |
| Kharchenko et al. | 2013 | 107.287 | -1.5 | â | 1.12 | -4.78 | â |
| Froebrich et al. | 2007 | 107.287 | -1.512 | â | â | â | â |
| Dias et al. | 2002 | 107.287 | -1.512 | â | 1.12 | -4.78 | 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 | 4.14 | 0.52 | 0.87 | 1369 | -0.256 | 239 | â | â |
| Li et al. | 2025 | 4.20 | 0.52 | â | 2235 | -0.306 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.160(5) | â | â | â |
| Almeida et al. | 2025 | 4.14 | 0.51 | â | 2203 | â | 168 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 239(1) | â | â |
| Cavallo et al. | 2024 | 3.68 | 0.70 | â | 1380 | -0.170 | â | â | â |
| Hunt & Reffert | 2023 | 4.70 | 0.29 | 0.87 | 1358 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 200 | â | 1285 | â | â |
| Dias et al. | 2021 | 4.14 | 0.51 | â | 2203 | -0.256 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.77 | 0.14 | â | 2754 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.300 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.53 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.53 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 5.80 | 1.74 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.80 | 1.74 | â | 200 | â | â | â | â |
| Dias et al. | 2002 | 5.80 | 1.74 | â | 200 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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