FSR 0923
(MWSC 777; MWSC 778)
0.78
UTI
0.69
CN
1.0
Cdens
0.5
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.69 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0923 is a moderately populated, very dense object of intermediate C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
Relatively close
High 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 | 92.648 | 16.975 | 0.585 | 0.535 | 0.164 | 42.967 |
| Zhang et al. | 2024 | 92.647 | 16.974 | â | â | â | â |
| Hunt & Reffert | 2024 | 92.647 | 16.974 | 0.568 | 0.512 | 0.151 | 36.564 |
| Cavallo et al. | 2024 | 92.646 | 16.95 | 0.57 | â | â | â |
| Hunt & Reffert | 2023 | 92.647 | 16.974 | 0.568 | 0.512 | 0.151 | 36.564 |
| Just et al. | 2023 | 92.632 | 16.971 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 92.644 | 16.971 | 0.587 | 0.657 | 0.141 | â |
| Cantat-Gaudin & Anders | 2020 | 92.644 | 16.971 | 0.587 | 0.657 | 0.141 | â |
| Soubiran et al. | 2018 | 92.644 | 16.971 | â | â | â | 43.83 |
| Bica et al. | 2019 | 92.649 | 16.97 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 92.644 | 16.971 | 0.587 | 0.657 | 0.141 | â |
| Loktin & Popova | 2017 | 92.64 | 16.981 | â | 0.228 | -1.762 | â |
| Kharchenko et al. | 2016 | 92.632 | 16.971 | â | â | â | â |
| Dias et al. | 2014 | 92.65 | 16.971 | â | -0.51 | 1.4 | â |
| Kharchenko et al. | 2013 | 92.64 | 16.97 | â | 0.83 | -6.51 | â |
| Froebrich et al. | 2007 | 92.65 | 16.971 | â | â | â | â |
| Dias et al. | 2002 | 92.65 | 16.971 | â | -0.51 | 1.4 | 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 | -0.181* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 591* | â | â |
| Cavallo et al. | 2024 | 1.79 | 3.09 | â | 372 | 0.430 | â | â | â |
| Hunt & Reffert | 2023 | 1.62 | 3.39 | 2.74 | 105 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 531 | â | 95 | â | â |
| Cantat-Gaudin et al. | 2020 | 1.67 | 1.84 | â | 977 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.62 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.62 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.62 | â | â | â | â | â | â | â |
| Loktin & Popova | 2017 | 2.02 | 3.34 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.44 | 3.87 | â | 531 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.44 | 3.87 | â | 531 | â | â | â | â |
| Dias et al. | 2002 | 1.50 | 4.19 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.