FSR 0519
(MWSC 83; FoF 550)
0.75
UTI
0.59
CN
0.77
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
3.9 [N/pc2]
- CN 0.59 Moderately populated
- Cdens 0.77 Dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0519 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster, but with a large variance across recent sources for the mass parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.94 kpc) differs significantly from the median photometric distance (~2.09 kpc).
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 13.155 | 64.628 | 0.34 | -2.433 | -0.379 | â |
| Hunt & Reffert | 2024 | 13.161 | 64.617 | 0.343 | -2.439 | -0.377 | -66.704 |
| Cavallo et al. | 2024 | 12.987 | 64.582 | 0.344 | â | â | â |
| Hunt & Reffert | 2023 | 13.161 | 64.617 | 0.343 | -2.439 | -0.377 | -66.704 |
| Just et al. | 2023 | 13.112 | 64.663 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 13.092 | 64.596 | 0.324 | -2.423 | -0.331 | â |
| Liu & Pang | 2019 | 13.179 | 64.618 | 0.35 | -2.437 | -0.276 | â |
| Cantat-Gaudin et al. | 2019 | 13.092 | 64.596 | 0.32 | -2.42 | -0.33 | â |
| Bica et al. | 2019 | 13.135 | 64.651 | â | â | â | â |
| Kharchenko et al. | 2016 | 13.112 | 64.663 | â | â | â | â |
| Kharchenko et al. | 2013 | 13.122 | 64.667 | â | 0.03 | 2.47 | â |
| Kharchenko et al. | 2012 | 13.122 | 64.667 | â | -0.68 | 1.43 | â |
| Froebrich et al. | 2007 | 13.125 | 64.651 | â | â | â | â |
| Dias et al. | 2002 | 13.125 | 64.651 | â | -5.38 | -2.55 | 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 | 2.09 | 2.17 | 1.92 | 38 | 0.345 | 508 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 947(1) | â | â |
| Cavallo et al. | 2024 | 2.86 | 2.38 | â | 60 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 2.66 | 2.36 | 1.92 | 53 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 22 | â | 69 | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.83 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 6 | 0.500 | â | â | â |
| Cantat-Gaudin et al. | 2019 | 2.83 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.52 | 2.16 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.52 | 2.16 | â | 22 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.45 | 2.17 | â | 1660 | â | â | â | â |
| Dias et al. | 2002 | 1.45 | 2.17 | â | 1660 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair P277, along with Casado_12.
Cavallo et al. (2024)
Gold sample.