FSR 0536
(SAI 13; MWSC 116)
0.78
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
11.9 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0536 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 19.92 | 63.052 | 0.277 | -1.639 | -0.128 | -47.636 |
| Hunt & Reffert | 2024 | 19.937 | 63.058 | 0.269 | -1.628 | -0.154 | -31.72 |
| Cavallo et al. | 2024 | 19.913 | 63.053 | 0.267 | â | â | â |
| Hunt & Reffert | 2023 | 19.937 | 63.058 | 0.269 | -1.628 | -0.154 | -31.72 |
| Just et al. | 2023 | 19.922 | 63.065 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 19.919 | 63.026 | 0.288 | -1.619 | -0.025 | â |
| Cantat-Gaudin & Anders | 2020 | 19.919 | 63.026 | 0.288 | -1.619 | -0.025 | â |
| Cantat-Gaudin et al. | 2018 | 19.919 | 63.026 | 0.288 | -1.619 | -0.025 | â |
| Kharchenko et al. | 2016 | 19.922 | 63.065 | â | â | â | â |
| Kharchenko et al. | 2013 | 19.933 | 63.067 | â | -1.16 | 1.98 | â |
| Kharchenko et al. | 2012 | 19.933 | 63.067 | â | -1.16 | 1.98 | â |
| Glushkova et al. | 2010 | 19.907 | 63.056 | â | â | â | â |
| Froebrich et al. | 2007 | 19.933 | 63.069 | â | â | â | â |
| Dias et al. | 2002 | 19.933 | 63.069 | â | 2.73 | 6.48 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.075 | 3.83 | 2.44 | 249 | 0.550 | 1571 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2413(1) | â | â |
| Cavallo et al. | 2024 | 4.55 | 4.30 | â | 34 | 0.550 | â | â | â |
| Hunt & Reffert | 2023 | 3.24 | 4.40 | 2.44 | 59 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 249 | â | 729 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.21 | 3.98 | â | 115 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.15 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.15 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.00 | 3.72 | â | 249 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.00 | 3.72 | â | 249 | â | â | â | â |
| Kharchenko et al. | 2012 | 3.00 | 3.72 | â | 249 | â | â | â | â |
| Glushkova et al. | 2010 | 3.00 | 3.94 | â | 158 | â | â | â | â |
| Dias et al. | 2002 | 3.00 | 3.72 | â | 249 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.