FSR 0951
(MWSC 849; FoF 1380)
0.91
UTI
0.81
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Radius (P>50% members)
9.0 [arcmin]
- CN 0.81 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0951 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 very well-studied in the literature.
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 | 95.565 | 14.65 | 0.564 | 0.214 | 0.03 | 43.986 |
| Li et al. | 2025 | 95.573 | 14.65 | 0.553 | 0.242 | 0.07 | â |
| Almeida et al. | 2025 | 95.591 | 14.636 | â | â | â | â |
| Zhang et al. | 2024 | 95.544 | 14.658 | â | â | â | â |
| Hunt & Reffert | 2024 | 95.544 | 14.658 | 0.562 | 0.226 | 0.013 | 42.078 |
| Cavallo et al. | 2024 | 95.573 | 14.625 | 0.564 | â | â | â |
| Hunt & Reffert | 2023 | 95.544 | 14.658 | 0.562 | 0.226 | 0.013 | 42.078 |
| Almeida et al. | 2023 | 95.596 | 14.628 | â | â | â | â |
| Just et al. | 2023 | 95.577 | 14.706 | â | â | â | â |
| Dias et al. | 2021 | 95.591 | 14.636 | 0.546 | 0.28 | 0.047 | 41.857 |
| Cantat-Gaudin et al. | 2020 | 95.573 | 14.65 | 0.553 | 0.242 | 0.07 | â |
| Cantat-Gaudin & Anders | 2020 | 95.573 | 14.65 | 0.553 | 0.242 | 0.07 | â |
| Liu & Pang | 2019 | 95.574 | 14.626 | 0.546 | 0.273 | -0.001 | â |
| Bossini et al. | 2019 | 95.573 | 14.65 | â | â | â | â |
| Soubiran et al. | 2018 | 95.573 | 14.65 | â | â | â | 45.53 |
| Bica et al. | 2019 | 95.585 | 14.712 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 95.573 | 14.65 | 0.553 | 0.242 | 0.07 | â |
| Kharchenko et al. | 2016 | 95.577 | 14.706 | â | â | â | â |
| Kharchenko et al. | 2013 | 95.584 | 14.705 | â | -0.26 | -0.84 | 42.0 |
| Froebrich et al. | 2007 | 95.579 | 14.712 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 1.78 | 1.02 | â | 472 | 0.148 | â | â | â |
| Almeida et al. | 2025 | 1.61 | 1.32 | â | 397 | â | 755 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.051* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 893* | â | â |
| Cavallo et al. | 2024 | 1.75 | 1.11 | â | 490 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.63 | 0.79 | 1.08 | 571 | â | â | â | â |
| Almeida et al. | 2023 | 1.58 | 1.21 | â | 619 | -0.110 | 916* | 0.45 | â |
| Just et al. | 2023 | â | â | â | 501 | â | 225 | â | â |
| Dias et al. | 2021 | 1.61 | 1.32 | â | 397 | -0.069 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.75 | 0.81 | â | 525 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.72 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 977 | -2.000 | â | â | â |
| Bossini et al. | 2019 | 2.10 | 1.15 | â | 388 | 0.000 | â | â | â |
| Soubiran et al. | 2018 | 1.72 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.72 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.62 | 1.48 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.62 | 1.48 | â | 501 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: good fit. Isochrone match: good fit. Gold sample.
Cavallo et al. (2024)
Gold sample.