FSR 0319
(MWSC 3560)
0.22
UTI
0.45
CN
0.05
Cdens
0.12
CC3
0.23
Clit
1.0
Cdup
Nm (P>50%)
45
Core radius and density
4.3 [pc], 0.3 [pc-2]
- CN 0.45 Poorly populated
- Cdens 0.05 Very loose
- CC3 0.12 Very low quality
- Clit 0.23 Rarely studied
- Cdup 1.0 Unique
Overview
FSR 0319 is a poorly populated, very loose object of very low C3 quality. Its parallax locates it at a moderate* distance, below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is rarely studied in the literature.
(*): The parallax distance estimate (~3.66 kpc) differs significantly from the median photometric distance (~1.68 kpc).
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 326.695 | 51.423 | 0.273 | -3.32 | -2.97 | -46.386 |
| Just et al. | 2023 | 326.635 | 51.415 | â | â | â | â |
| Bica et al. | 2019 | 326.65 | 51.41 | â | â | â | â |
| Dib et al. | 2018 | 326.64 | 51.418 | â | â | â | â |
| Joshi et al. | 2016 | 326.64 | 51.418 | â | â | â | â |
| Kharchenko et al. | 2016 | 326.635 | 51.415 | â | â | â | â |
| Kharchenko et al. | 2013 | 326.64 | 51.418 | â | -4.01 | -3.13 | â |
| Kharchenko et al. | 2012 | 326.64 | 51.418 | â | -4.01 | -3.13 | â |
| Froebrich et al. | 2007 | 326.65 | 51.412 | â | â | â | â |
| Dias et al. | 2002 | 326.65 | 51.412 | â | -4.01 | -3.13 | 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 | 1.68 | 2.68 | â | 398 | â | 90 | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 90 | â | â |
| Dib et al. | 2018 | 1.68 | â | â | 398 | â | â | â | â |
| Joshi et al. | 2016 | 1.68 | 2.68 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.68 | 2.68 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.68 | 2.68 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.68 | 2.68 | â | 398 | â | â | â | â |
| Dias et al. | 2002 | 1.68 | 2.68 | â | 398 | â | â | â | â |
MOCA
