FSR 1591
(MWSC 1959)
0.67
UTI
0.35
CN
0.85
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.35 Poorly populated
- Cdens 0.85 Dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1591 is a poorly populated, dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Distant
High extinction
Metal-poor
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 174.269 | -62.726 | 0.233 | -5.508 | 1.62 | -7.324 |
| Hunt & Reffert | 2024 | 174.258 | -62.737 | 0.224 | -5.612 | 1.462 | -13.822 |
| Cavallo et al. | 2024 | 174.264 | -62.728 | 0.211 | â | â | â |
| Hunt & Reffert | 2023 | 174.258 | -62.737 | 0.224 | -5.612 | 1.462 | -13.822 |
| Just et al. | 2023 | 174.232 | -62.719 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 174.222 | -62.731 | 0.255 | -5.469 | 1.67 | â |
| Cantat-Gaudin & Anders | 2020 | 174.222 | -62.731 | 0.255 | -5.469 | 1.67 | â |
| Soubiran et al. | 2018 | 174.222 | -62.731 | â | â | â | -10.27 |
| Bica et al. | 2019 | 174.232 | -62.748 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 174.222 | -62.731 | 0.255 | -5.469 | 1.67 | â |
| Kharchenko et al. | 2016 | 174.232 | -62.719 | â | â | â | â |
| Kharchenko et al. | 2013 | 174.24 | -62.723 | â | -7.66 | 0.46 | â |
| Froebrich et al. | 2007 | 174.238 | -62.744 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1356* | â | â |
| Cavallo et al. | 2024 | 4.81 | 5.08 | â | 138 | -0.560 | â | â | â |
| Hunt & Reffert | 2023 | 3.88 | 4.92 | 2.62 | 182 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 501 | â | 83 | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.52 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.52 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.52 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.54 | 2.55 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.54 | 2.55 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.