FSR 0542
(MWSC 119)
0.83
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.81
Clit
1.0
Cdup
Stellar density (N50/rad)
8.8 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.81 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0542 is a rich, very dense object of 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, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 21.474 | 63.003 | 0.255 | -2.157 | -0.288 | -72.772 |
| Hunt & Reffert | 2024 | 21.459 | 62.994 | 0.255 | -2.145 | -0.329 | -72.054 |
| Cavallo et al. | 2024 | 21.45 | 62.995 | 0.252 | â | â | â |
| Hunt & Reffert | 2023 | 21.459 | 62.994 | 0.255 | -2.145 | -0.329 | -72.054 |
| Just et al. | 2023 | 21.439 | 62.981 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 21.485 | 63.011 | 0.271 | -2.187 | -0.203 | â |
| Donor et al. | 2020 | 21.45 | 62.985 | â | -2.09 | -0.11 | -74.0 |
| Cantat-Gaudin & Anders | 2020 | 21.485 | 63.011 | 0.271 | -2.187 | -0.203 | â |
| Soubiran et al. | 2018 | 21.485 | 63.011 | â | â | â | -63.93 |
| Cantat-Gaudin et al. | 2018 | 21.485 | 63.011 | 0.271 | -2.187 | -0.203 | â |
| Kharchenko et al. | 2016 | 21.439 | 62.981 | â | â | â | â |
| Dias et al. | 2014 | 21.471 | 62.995 | â | -1.38 | -0.08 | â |
| Kharchenko et al. | 2013 | 21.45 | 62.985 | â | 1.22 | -2.31 | â |
| Kharchenko et al. | 2012 | 21.45 | 62.985 | â | 1.22 | -2.31 | â |
| Froebrich et al. | 2007 | 21.471 | 62.995 | â | â | â | â |
| Dias et al. | 2002 | 21.471 | 62.995 | â | -1.38 | -0.08 | 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 | 3.245 | 2.58 | 2.75 | 224 | -0.080 | 667 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1225(1) | â | â |
| Cavallo et al. | 2024 | 3.21 | 4.00 | â | 224 | -0.080 | â | â | â |
| Hunt & Reffert | 2023 | 3.28 | 3.37 | 2.75 | 34 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 224 | â | 109 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.75 | 3.24 | â | 851 | â | â | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.230 | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.33 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 3.33 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.33 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.93 | 2.58 | â | 224 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.93 | 2.58 | â | 224 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.93 | 2.58 | â | 224 | â | â | â | â |
| Dias et al. | 2002 | 1.93 | 2.58 | â | 224 | 0.070 | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Wood sample.