FSR 1275
(SAI 77; MWSC 1233)
0.57
UTI
0.3
CN
1.0
Cdens
0.25
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.3 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.25 Low quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1275 is a poorly populated, very dense object of low 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, old cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.37 kpc) differs significantly from the median photometric distance (~3.75 kpc).
Distant
Moderate extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 112.032 | -21.785 | 0.422 | -2.142 | 2.195 | â |
| Hunt & Reffert | 2024 | 112.02 | -21.771 | 0.424 | -2.125 | 2.208 | â |
| Cavallo et al. | 2024 | 112.047 | -21.748 | 0.423 | â | â | â |
| Hunt & Reffert | 2023 | 112.02 | -21.771 | 0.424 | -2.125 | 2.208 | â |
| Just et al. | 2023 | 112.007 | -21.788 | â | â | â | â |
| Bica et al. | 2019 | 112.026 | -21.8 | â | â | â | â |
| Kharchenko et al. | 2016 | 112.007 | -21.788 | â | â | â | â |
| Dias et al. | 2014 | 112.025 | -21.796 | â | -1.79 | 0.06 | â |
| Kharchenko et al. | 2013 | 112.012 | -21.79 | â | -2.91 | 2.71 | â |
| Glushkova et al. | 2010 | 112.026 | -21.796 | â | â | â | â |
| Froebrich et al. | 2007 | 112.021 | -21.796 | â | â | â | â |
| Dias et al. | 2002 | 112.025 | -21.796 | â | -1.79 | 0.06 | 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 | 380* | â | â |
| Cavallo et al. | 2024 | 2.57 | 1.60 | â | 29 | 0.220 | â | â | â |
| Hunt & Reffert | 2023 | 2.17 | 1.12 | 1.02 | 26 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 2512 | â | 5483 | â | â |
| Kharchenko et al. | 2016 | 4.54 | 2.06 | â | 2512 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.54 | 2.06 | â | 2512 | â | â | â | â |
| Glushkova et al. | 2010 | 3.75 | 1.86 | â | 2512 | â | â | â | â |
| Dias et al. | 2002 | 3.75 | 1.86 | â | 2512 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.