FSR 0921
(SAI 58; MWSC 727)
0.77
UTI
0.76
CN
1.0
Cdens
0.5
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
4.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0921 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, below 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 metallicity parameter (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 | 91.308 | 16.677 | 0.358 | 0.054 | -1.6 | 13.757 |
| Zhang et al. | 2024 | 91.293 | 16.688 | â | â | â | â |
| Hunt & Reffert | 2024 | 91.293 | 16.688 | 0.355 | 0.011 | -1.569 | 24.107 |
| Cavallo et al. | 2024 | 91.32 | 16.664 | 0.35 | â | â | â |
| Hunt & Reffert | 2023 | 91.293 | 16.688 | 0.355 | 0.011 | -1.569 | 24.107 |
| Just et al. | 2023 | 91.312 | 16.676 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 91.295 | 16.684 | 0.327 | -0.006 | -1.652 | â |
| Cantat-Gaudin & Anders | 2020 | 91.295 | 16.684 | 0.327 | -0.006 | -1.652 | â |
| Soubiran et al. | 2018 | 91.295 | 16.684 | â | â | â | 29.57 |
| Bica et al. | 2019 | 91.287 | 16.681 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 91.295 | 16.684 | 0.327 | -0.006 | -1.652 | â |
| Kharchenko et al. | 2016 | 91.312 | 16.676 | â | â | â | â |
| Kharchenko et al. | 2013 | 91.32 | 16.675 | â | 2.55 | -7.92 | â |
| Glushkova et al. | 2010 | 91.289 | 16.684 | â | â | â | â |
| Froebrich et al. | 2007 | 91.321 | 16.678 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.096* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1364* | â | â |
| Cavallo et al. | 2024 | 2.74 | 4.09 | â | 245 | 0.460 | â | â | â |
| Hunt & Reffert | 2023 | 2.35 | 4.00 | 2.82 | 221 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 562 | â | 188 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.27 | 3.22 | â | 389 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.81 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.81 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.81 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.81 | 3.00 | â | 562 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.81 | 3.00 | â | 562 | â | â | â | â |
| Glushkova et al. | 2010 | 2.29 | 4.12 | â | 316 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.