FSR 0344
(MWSC 3580)
0.82
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.3 [arcmin]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0344 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, near 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 metallicity parameter (see Parameters). It is well-studied in the literature.
Distant
Moderate extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 330.449 | 54.8 | 0.198 | -1.741 | -1.622 | -58.191 |
| Hu & Soubiran | 2025 | 330.448 | 54.807 | â | â | â | â |
| Hunt & Reffert | 2024 | 330.434 | 54.802 | 0.202 | -1.741 | -1.608 | -57.398 |
| Cavallo et al. | 2024 | 330.448 | 54.807 | 0.204 | â | â | â |
| Hunt & Reffert | 2023 | 330.434 | 54.802 | 0.202 | -1.741 | -1.608 | -57.398 |
| Just et al. | 2023 | 330.424 | 54.821 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 330.44 | 54.815 | 0.196 | -1.792 | -1.591 | â |
| Cantat-Gaudin & Anders | 2020 | 330.44 | 54.815 | 0.196 | -1.792 | -1.591 | â |
| Soubiran et al. | 2018 | 330.44 | 54.815 | â | â | â | -63.41 |
| Bica et al. | 2019 | 330.419 | 54.817 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 330.44 | 54.815 | 0.196 | -1.792 | -1.591 | â |
| Kharchenko et al. | 2016 | 330.424 | 54.821 | â | â | â | â |
| Kharchenko et al. | 2013 | 330.43 | 54.825 | â | -4.98 | -3.23 | â |
| Kharchenko et al. | 2012 | 330.43 | 54.825 | â | -4.98 | -3.23 | â |
| Froebrich et al. | 2007 | 330.413 | 54.819 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.090* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1695* | â | â |
| Cavallo et al. | 2024 | 4.94 | 3.63 | â | 832 | -0.560 | â | â | â |
| Hunt & Reffert | 2023 | 4.21 | 3.56 | 2.25 | 1096 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 794 | â | 36 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.41 | 3.04 | â | 3467 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.45 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.45 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.45 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.30 | 2.23 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 2.23 | â | 794 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.30 | 2.23 | â | 794 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.