FSR 1170
(MWSC 1111)
0.74
UTI
0.67
CN
1.0
Cdens
0.38
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.67 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1170 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 | β | 106.867 | -8.87 | 0.334 | -0.682 | -0.171 | 42.608 |
| Almeida et al. | 2025 | 106.87 | -8.876 | β | β | β | β |
| Hunt & Reffert | 2024 | 106.872 | -8.872 | 0.34 | -0.686 | -0.144 | 42.608 |
| Cavallo et al. | 2024 | 106.856 | -8.867 | 0.345 | β | β | β |
| Hunt & Reffert | 2023 | 106.872 | -8.872 | 0.34 | -0.686 | -0.144 | 42.608 |
| Just et al. | 2023 | 106.868 | -8.863 | β | β | β | β |
| Dias et al. | 2021 | 106.87 | -8.876 | 0.331 | -0.643 | -0.201 | β |
| Cantat-Gaudin et al. | 2020 | 106.873 | -8.879 | 0.33 | -0.639 | -0.213 | β |
| SΓ‘nchez et al. | 2020 | 106.862 | -8.867 | β | -0.541 | -0.123 | β |
| Cantat-Gaudin & Anders | 2020 | 106.873 | -8.879 | 0.33 | -0.639 | -0.213 | β |
| Soubiran et al. | 2018 | 106.873 | -8.879 | β | β | β | 42.84 |
| Cantat-Gaudin et al. | 2018 | 106.873 | -8.879 | 0.33 | -0.639 | -0.213 | β |
| Kharchenko et al. | 2016 | 106.868 | -8.863 | β | β | β | β |
| Kharchenko et al. | 2013 | 106.875 | -8.865 | β | 7.48 | -1.65 | β |
| Froebrich et al. | 2007 | 106.862 | -8.867 | β | β | β | β |
| Dias et al. | 2002 | 106.862 | -8.867 | β | 0.83 | -1.82 | β |
π‘ 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 | 2.69 | 2.33 | β | 328 | β | 227 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 578* | β | β |
| Cavallo et al. | 2024 | 2.88 | 2.67 | β | 229 | -0.110 | β | β | β |
| Hunt & Reffert | 2023 | 2.54 | 2.02 | 1.98 | 324 | β | β | β | β |
| Just et al. | 2023 | β | β | β | 569 | β | 192 | β | β |
| Dias et al. | 2021 | 2.69 | 2.33 | β | 328 | 0.136 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.10 | 1.85 | β | 195 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.79 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 2.79 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.79 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.28 | 2.06 | β | 569 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.28 | 2.06 | β | 569 | β | β | β | β |
| Dias et al. | 2002 | 2.28 | 2.06 | β | 569 | β | β | β | β |
(*): 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.