FSR 1197
(MWSC 1015)
0.60
UTI
0.74
CN
0.62
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
3.1 [N/pc2]
- CN 0.74 Moderately populated
- Cdens 0.62 Moderately dense
- CC3 0.75 High quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1197 is a moderately populated, moderately dense object of high C3 quality. Its parallax locates it at a close* distance, below 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 parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~0.85 kpc) differs significantly from the median photometric distance (~1.24 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 103.671 | -13.861 | 1.175 | -3.039 | -0.716 | 25.707 |
| Hunt & Reffert | 2024 | 103.591 | -13.748 | 1.151 | -3.046 | -0.709 | 26.929 |
| Cavallo et al. | 2024 | 103.596 | -13.882 | 1.165 | â | â | â |
| Hunt & Reffert | 2023 | 103.591 | -13.748 | 1.151 | -3.046 | -0.709 | 26.929 |
| Just et al. | 2023 | 103.618 | -13.657 | â | â | â | â |
| Bica et al. | 2019 | 103.63 | -13.656 | â | â | â | â |
| Kharchenko et al. | 2016 | 103.618 | -13.657 | â | â | â | â |
| Kharchenko et al. | 2013 | 103.624 | -13.658 | â | 2.36 | -2.17 | â |
| Froebrich et al. | 2007 | 103.625 | -13.658 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.24 | 0.83 | 0.64 | 1000 | 0.120 | 126 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 198(1) | â | â |
| Cavallo et al. | 2024 | 0.85 | 0.37 | â | 182 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 0.81 | 0.14 | 0.64 | 146 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1000 | â | 53 | â | â |
| Kharchenko et al. | 2016 | 1.63 | 1.29 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.63 | 1.29 | â | 1000 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.