FSR 0948
(SAI 64; MWSC 867)
0.90
UTI
0.75
CN
1.0
Cdens
0.75
CC3
1.0
Clit
1.0
Cdup
Stellar density (N50/rad)
9.1 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 1.0 Very well-studied
- Cdup 1.0 Unique
Overview
FSR 0948 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above 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.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 96.49 | 15.858 | 0.218 | -0.152 | 0.053 | 52.077 |
| Li et al. | 2025 | 96.48 | 15.859 | 0.2 | -0.132 | 0.051 | β |
| Almeida et al. | 2025 | 96.476 | 15.868 | β | β | β | β |
| Zhang et al. | 2024 | 96.483 | 15.855 | β | β | β | β |
| Hunt & Reffert | 2024 | 96.483 | 15.855 | 0.22 | -0.151 | 0.046 | 44.467 |
| Cavallo et al. | 2024 | 96.481 | 15.863 | 0.22 | β | β | β |
| Hunt & Reffert | 2023 | 96.483 | 15.855 | 0.22 | -0.151 | 0.046 | 44.467 |
| Almeida et al. | 2023 | 96.479 | 15.865 | β | β | β | β |
| Just et al. | 2023 | 96.46 | 15.861 | β | β | β | β |
| Dias et al. | 2021 | 96.476 | 15.868 | 0.202 | -0.113 | 0.045 | β |
| Cantat-Gaudin et al. | 2020 | 96.48 | 15.859 | 0.2 | -0.132 | 0.051 | β |
| SΓ‘nchez et al. | 2020 | 96.471 | 15.861 | β | -0.197 | 0.024 | β |
| Zhong et al. | 2020 | 96.48 | 15.859 | β | -0.132 | 0.051 | 49.688 |
| Cantat-Gaudin & Anders | 2020 | 96.48 | 15.859 | 0.2 | -0.132 | 0.051 | β |
| Soubiran et al. | 2018 | 96.48 | 15.859 | β | β | β | 49.22 |
| Bica et al. | 2019 | 96.495 | 15.855 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 96.48 | 15.859 | 0.2 | -0.132 | 0.051 | β |
| Kharchenko et al. | 2016 | 96.46 | 15.861 | β | β | β | β |
| Dias et al. | 2014 | 96.471 | 15.861 | β | 0.42 | -0.94 | β |
| Kharchenko et al. | 2013 | 96.468 | 15.86 | β | -0.48 | -4.27 | β |
| Glushkova et al. | 2010 | 96.483 | 15.861 | β | β | β | β |
| Froebrich et al. | 2007 | 96.496 | 15.852 | β | β | β | β |
| Dias et al. | 2002 | 96.471 | 15.861 | β | 0.42 | -0.94 | β |
π‘ 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999β | 3.63 | 1.21 | 0.8 | 537 | -0.198 | 362 | 0.59 | β |
| Li et al. | 2025 | 4.05 | 1.59 | β | 536 | -0.032 | β | β | β |
| Almeida et al. | 2025 | 3.42 | 1.77 | β | 494 | β | 374 | β | β |
| Zhang et al. | 2024 | β | β | β | β | -0.226(1) | β | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 596(1) | β | β |
| Cavallo et al. | 2024 | 3.63 | 1.90 | β | 275 | -0.190 | β | β | β |
| Hunt & Reffert | 2023 | 3.98 | 1.18 | 0.80 | 486 | β | β | β | β |
| Almeida et al. | 2023 | 3.63 | 1.74 | β | 448 | -0.205 | 351(1) | 0.59 | β |
| Just et al. | 2023 | β | β | β | 603 | β | 340 | β | β |
| Dias et al. | 2021 | 3.42 | 1.77 | β | 494 | -0.255 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 4.09 | 1.24 | β | 537 | β | β | β | β |
| Zhong et al. | 2020 | 2.99 | 1.16 | β | 8780 | 0.000 | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 4.36 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 4.36 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 4.36 | β | β | β | β | β | β | β |
| Kharchenko et al. | 2016 | 2.99 | 1.16 | β | 603 | β | β | β | β |
| Kharchenko et al. | 2013 | 2.99 | 1.16 | β | 603 | β | β | β | β |
| Glushkova et al. | 2010 | 2.33 | 0.25 | β | 1000 | β | β | β | β |
| Dias et al. | 2002 | 2.33 | 0.25 | β | 1000 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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