FSR 0717
0.60
UTI
0.76
CN
1.0
Cdens
0.38
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
4.7 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0717 is a rich, 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 near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
Distant
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 | â | 71.503 | 42.145 | 0.268 | 0.081 | -1.158 | -12.638 |
| Hunt & Reffert | 2024 | 71.504 | 42.158 | 0.258 | 0.058 | -1.136 | â |
| Cavallo et al. | 2024 | 71.507 | 42.151 | 0.258 | â | â | â |
| He et al. | 2023 | 71.51 | 42.156 | 0.268 | 0.072 | -1.165 | -1.14 |
| Hunt & Reffert | 2023 | 71.504 | 42.158 | 0.258 | 0.058 | -1.136 | â |
| Dias et al. | 2014 | 71.525 | 42.134 | â | -2.35 | 1.13 | â |
| Froebrich et al. | 2007 | 71.525 | 42.134 | â | â | â | â |
| Dias et al. | 2002 | 71.525 | 42.134 | â | -3.13 | -1.48 | 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 | 494* | â | â |
| Cavallo et al. | 2024 | 3.70 | 2.30 | â | 78 | 0.430 | â | â | â |
| He et al. | 2023 | 3.47 | 2.25 | â | 158 | â | â | â | â |
| Hunt & Reffert | 2023 | 3.48 | 2.30 | 1.04 | 73 | â | â | â | â |
| Dias et al. | 2002 | 1.70 | 1.40 | â | 1122 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.