FSR 0723
(MWSC 414)
0.45
UTI
0.36
CN
0.37
Cdens
0.62
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.36 Poorly populated
- Cdens 0.37 Loose
- CC3 0.62 Intermediate quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0723 is a poorly populated, loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a small percentage of members with 2 later reported entries. See table with shared members information.
Relatively close
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 | 71.225 | 41.528 | 0.296 | -0.063 | -1.235 | -3.82 |
| Zhang et al. | 2024 | 71.233 | 41.519 | â | â | â | â |
| Hunt & Reffert | 2024 | 71.233 | 41.519 | 0.298 | 0.004 | -1.232 | â |
| Cavallo et al. | 2024 | 71.291 | 41.549 | 0.299 | â | â | â |
| Hunt & Reffert | 2023 | 71.233 | 41.519 | 0.298 | 0.004 | -1.232 | â |
| Bica et al. | 2019 | 71.243 | 41.516 | â | â | â | â |
| Froebrich et al. | 2007 | 71.237 | 41.513 | â | â | â | â |
| Dias et al. | 2002 | 71.237 | 41.513 | â | 0.13 | -0.17 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.031* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 405* | â | â |
| Cavallo et al. | 2024 | 2.96 | 1.56 | â | 95 | -0.310 | â | â | â |
| Hunt & Reffert | 2023 | 2.98 | 1.21 | 1.18 | 151 | â | â | â | â |
| Dias et al. | 2002 | 3.10 | 2.33 | â | 923 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.