FSR 0817
(MWSC 622)
0.74
UTI
0.76
CN
1.0
Cdens
0.62
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
5.3 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0817 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, old cluster (see Parameters). It is moderately studied in the literature.
Note: This object shares a moderate percentage of members with a later reported entry. See table with shared members information.
Relatively close
Moderate extinction
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 84.861 | 30.886 | 0.675 | -0.193 | -3.165 | 0.337 |
| Zhang et al. | 2024 | 84.86 | 30.89 | â | â | â | â |
| Hunt & Reffert | 2024 | 84.86 | 30.89 | 0.683 | -0.165 | -3.177 | -3.346 |
| Cavallo et al. | 2024 | 84.851 | 30.845 | 0.693 | â | â | â |
| Hunt & Reffert | 2023 | 84.86 | 30.89 | 0.683 | -0.165 | -3.177 | -3.346 |
| Just et al. | 2023 | 84.855 | 30.904 | â | â | â | â |
| Kharchenko et al. | 2016 | 84.855 | 30.904 | â | â | â | â |
| Dias et al. | 2014 | 84.862 | 30.893 | â | -0.78 | -5.9 | 25.0 |
| Kharchenko et al. | 2013 | 84.864 | 30.903 | â | 3.02 | -6.98 | â |
| Kharchenko et al. | 2012 | 84.864 | 30.903 | â | 3.02 | -6.98 | â |
| Froebrich et al. | 2007 | 84.862 | 30.893 | â | â | â | â |
| Dias et al. | 2002 | 84.862 | 30.893 | â | -0.78 | -5.9 | 25.0 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | 0.080* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 331* | â | â |
| Cavallo et al. | 2024 | 1.36 | 1.29 | â | 8 | 0.110 | â | â | â |
| Hunt & Reffert | 2023 | 1.34 | 1.26 | 1.47 | 7 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1122 | â | 36 | â | â |
| Kharchenko et al. | 2016 | 1.36 | 1.29 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.36 | 1.29 | â | 1122 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.36 | 1.29 | â | 1122 | â | â | â | â |
| Dias et al. | 2002 | 1.36 | 1.29 | 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.