FSR 0937
(MWSC 800)
0.89
UTI
0.68
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0937 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is very well-studied in the literature.
Very 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 | 93.423 | 14.996 | 0.157 | 0.376 | -0.139 | 19.007 |
| Hu & Soubiran | 2025 | 93.524 | 14.96 | â | â | â | â |
| Almeida et al. | 2025 | 93.433 | 15.008 | â | â | â | â |
| Zhang et al. | 2024 | 93.419 | 14.997 | â | â | â | â |
| Hunt & Reffert | 2024 | 93.419 | 14.997 | 0.189 | 0.402 | -0.229 | 31.266 |
| Cavallo et al. | 2024 | 93.524 | 14.96 | 0.19 | â | â | â |
| Hunt & Reffert | 2023 | 93.419 | 14.997 | 0.189 | 0.402 | -0.229 | 31.266 |
| Just et al. | 2023 | 93.418 | 14.996 | â | â | â | â |
| Dias et al. | 2021 | 93.433 | 15.008 | 0.08 | 0.549 | -0.13 | â |
| Cantat-Gaudin et al. | 2020 | 93.425 | 15.006 | 0.085 | 0.5 | -0.114 | â |
| Cantat-Gaudin & Anders | 2020 | 93.425 | 15.006 | 0.085 | 0.5 | -0.114 | â |
| Soubiran et al. | 2018 | 93.425 | 15.006 | â | â | â | 18.18 |
| Bica et al. | 2019 | 93.419 | 14.993 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 93.425 | 15.006 | 0.085 | 0.5 | -0.114 | â |
| Kharchenko et al. | 2016 | 93.418 | 14.996 | â | â | â | â |
| Kharchenko et al. | 2013 | 93.426 | 14.995 | â | -0.08 | -1.78 | â |
| Froebrich et al. | 2007 | 93.421 | 14.996 | â | â | â | â |
| Dias et al. | 2002 | 93.421 | 14.996 | â | -0.08 | -1.78 | 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 | -0.270* | â | â | â |
| Almeida et al. | 2025 | 5.58 | 2.33 | â | 1038 | â | 282 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.216* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 954* | â | â |
| Cavallo et al. | 2024 | 4.47 | 2.33 | â | 741 | -0.170 | â | â | â |
| Hunt & Reffert | 2023 | 4.78 | 2.17 | 2.15 | 555 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 955 | â | 912 | â | â |
| Dias et al. | 2021 | 5.58 | 2.33 | â | 1038 | -0.334 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 7.69 | 1.59 | â | 1202 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 8.80 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 8.80 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 8.80 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.60 | 1.81 | â | 955 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.60 | 1.81 | â | 955 | â | â | â | â |
| Dias et al. | 2002 | 4.60 | 1.81 | â | 955 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.