FSR 0816
(MWSC 620)
0.24
UTI
0.0
CN
0.09
Cdens
0.12
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
5.6 [arcmin]
- CN 0.0 Sparse
- Cdens 0.09 Very loose
- CC3 0.12 Very low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0816 is a sparse, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, near-solar metallicity, young cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~4.00 kpc) differs significantly from the median photometric distance (~2.16 kpc).
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.
Relatively close
High extinction
Low mass
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 84.747 | 31.498 | 0.25 | -0.324 | -1.699 | â |
| Just et al. | 2023 | 84.823 | 31.517 | â | â | â | â |
| Donor et al. | 2020 | 84.832 | 31.516 | â | 0.9 | -3.32 | -18.4 |
| Bica et al. | 2019 | 84.824 | 31.501 | â | â | â | â |
| Kharchenko et al. | 2016 | 84.823 | 31.517 | â | â | â | â |
| Kharchenko et al. | 2013 | 84.832 | 31.516 | â | 1.4 | -8.85 | â |
| Kharchenko et al. | 2012 | 84.832 | 31.516 | â | 1.32 | -8.34 | â |
| Froebrich et al. | 2007 | 84.821 | 31.501 | â | â | â | â |
| Dias et al. | 2002 | 84.821 | 31.501 | â | 1.32 | -8.34 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 63 | â | 45 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.100 | â | â | â |
| Kharchenko et al. | 2016 | 2.22 | 3.55 | â | 63 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.22 | 3.55 | â | 63 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.10 | 3.10 | â | 562 | â | â | â | â |
| Dias et al. | 2002 | 2.10 | 3.10 | â | 562 | â | â | â | â |
