FSR 0442
(MWSC 3732)
0.85
UTI
0.87
CN
1.0
Cdens
0.75
CC3
0.82
Clit
1.0
Cdup
Radius (P>50% members)
8.2 [arcmin]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.82 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0442 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, metal-rich, old cluster (see Parameters). It is well-studied in the literature.
Relatively close
High extinction
Massive
Metal-rich
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 352.486 | 63.447 | 0.688 | 1.26 | -2.55 | -26.247 |
| Hunt & Reffert | 2024 | 352.494 | 63.447 | 0.684 | 1.269 | -2.562 | -15.331 |
| Cavallo et al. | 2024 | 352.462 | 63.455 | 0.685 | â | â | â |
| Hunt & Reffert | 2023 | 352.494 | 63.447 | 0.684 | 1.269 | -2.562 | -15.331 |
| Just et al. | 2023 | 352.492 | 63.431 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 352.489 | 63.447 | 0.664 | 1.287 | -2.554 | â |
| Cantat-Gaudin & Anders | 2020 | 352.489 | 63.447 | 0.664 | 1.287 | -2.554 | â |
| Soubiran et al. | 2018 | 352.489 | 63.447 | â | â | â | -27.24 |
| Bica et al. | 2019 | 352.502 | 63.479 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 352.489 | 63.447 | 0.664 | 1.287 | -2.554 | â |
| Kharchenko et al. | 2016 | 352.492 | 63.431 | â | â | â | â |
| Dias et al. | 2014 | 352.508 | 63.482 | â | 1.44 | 0.56 | â |
| Kharchenko et al. | 2013 | 352.5 | 63.435 | â | -0.49 | -4.09 | â |
| Kharchenko et al. | 2012 | 352.5 | 63.435 | â | -0.49 | -4.09 | â |
| Froebrich et al. | 2007 | 352.508 | 63.482 | â | â | â | â |
| Dias et al. | 2002 | 352.508 | 63.482 | â | 1.44 | 0.56 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 2322* | â | â |
| Cavallo et al. | 2024 | 1.45 | 3.38 | â | 676 | 0.550 | â | â | â |
| Hunt & Reffert | 2023 | 1.39 | 3.56 | 2.68 | 395 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1000 | â | 53 | â | â |
| Cantat-Gaudin et al. | 2020 | 1.71 | 2.44 | â | 741 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.44 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.44 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.44 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.25 | 4.45 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.25 | 4.45 | â | 1000 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.25 | 4.45 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 1.25 | 4.45 | â | 1000 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.