FSR 1017
(MWSC 567)
0.36
UTI
0.25
CN
0.93
Cdens
0.12
CC3
0.25
Clit
1.0
Cdup
Radius (P>50% members)
230.6 [arcmin]
- CN 0.25 Poorly populated
- Cdens 0.93 Very dense
- CC3 0.12 Very low quality
- Clit 0.25 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1017 is a poorly populated, very dense object of very low C3 quality. Its parallax locates it at a very close distance, near the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is poorly studied in the literature.
Very close
Low extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 81.152 | -3.06 | 28.969 | 16.915 | -51.792 | 21.628 |
| Cavallo et al. | 2024 | 79.875 | -1.981 | 30.919 | â | â | â |
| Hunt & Reffert | 2023 | 82.969 | -3.035 | 30.919 | 17.945 | -61.139 | 32.183 |
| Bica et al. | 2019 | 83.036 | -3.039 | â | â | â | â |
| Froebrich et al. | 2007 | 83.037 | -3.038 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Cavallo et al. | 2024 | 0.04 | 0.68 | â | 62 | -0.220 | â | â | â |
| Hunt & Reffert | 2023 | 0.04 | 0.38 | 0.51 | 16 | â | â | â | â |
Cavallo et al. (2024)
Bronze sample.
Hunt & Reffert (2024)
Classified as a moving group.