FSR 1183
(MWSC 1144)
0.70
UTI
0.64
CN
1.0
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
2.5 [arcmin]
- CN 0.64 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1183 is a moderately populated, very dense object of low C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (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 | 108.357 | -9.889 | 0.415 | -1.44 | 1.237 | â |
| Li et al. | 2025 | 108.357 | -9.884 | 0.428 | -1.419 | 1.217 | â |
| Hunt & Reffert | 2024 | 108.354 | -9.891 | 0.424 | -1.434 | 1.251 | â |
| Cavallo et al. | 2024 | 108.36 | -9.883 | 0.429 | â | â | â |
| Hunt & Reffert | 2023 | 108.354 | -9.891 | 0.424 | -1.434 | 1.251 | â |
| Just et al. | 2023 | 108.332 | -9.89 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 108.357 | -9.884 | 0.428 | -1.419 | 1.217 | â |
| Cantat-Gaudin & Anders | 2020 | 108.357 | -9.884 | 0.428 | -1.419 | 1.217 | â |
| Cantat-Gaudin et al. | 2018 | 108.357 | -9.884 | 0.428 | -1.419 | 1.217 | â |
| Kharchenko et al. | 2016 | 108.332 | -9.89 | â | â | â | â |
| Dias et al. | 2014 | 108.342 | -9.872 | â | -2.9 | -3.22 | â |
| Kharchenko et al. | 2013 | 108.339 | -9.892 | â | -1.47 | -0.57 | â |
| Froebrich et al. | 2007 | 108.342 | -9.872 | â | â | â | â |
| Dias et al. | 2002 | 108.342 | -9.872 | â | -2.9 | -3.22 | 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 | 2.05 | 1.03 | â | 271 | -0.066 | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 210* | â | â |
| Cavallo et al. | 2024 | 1.96 | 1.16 | â | 251 | -0.130 | â | â | â |
| Hunt & Reffert | 2023 | 2.12 | 0.95 | 1.26 | 309 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 385 | â | 280 | â | â |
| Cantat-Gaudin et al. | 2020 | 2.20 | 0.40 | â | 182 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.19 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.19 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.63 | 1.29 | â | 385 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.63 | 1.29 | â | 385 | â | â | â | â |
| Dias et al. | 2002 | 1.63 | 1.29 | â | 385 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.