FSR 0674
(MWSC 350)
0.70
UTI
0.61
CN
1.0
Cdens
0.38
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
8.7 [N/pc2]
- CN 0.61 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.38 Low quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0674 is a moderately populated, very dense object of low 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.
Note: This object shares a large percentage of members with 2 later reported entries. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 63.096 | 48.729 | 0.324 | -0.965 | -0.785 | -28.953 |
| Almeida et al. | 2025 | 63.098 | 48.73 | â | â | â | â |
| Zhang et al. | 2024 | 63.106 | 48.726 | â | â | â | â |
| Hunt & Reffert | 2024 | 63.106 | 48.726 | 0.331 | -0.95 | -0.801 | -13.086 |
| Cavallo et al. | 2024 | 63.096 | 48.722 | 0.333 | â | â | â |
| He et al. | 2023 | 63.1 | 48.728 | 0.333 | -0.976 | -0.781 | -13.09 |
| Hunt & Reffert | 2023 | 63.106 | 48.726 | 0.331 | -0.95 | -0.801 | -13.086 |
| Just et al. | 2023 | 63.083 | 48.728 | â | â | â | â |
| Dias et al. | 2021 | 63.098 | 48.73 | 0.275 | -0.894 | -0.871 | â |
| Bica et al. | 2019 | 63.086 | 48.733 | â | â | â | â |
| Kharchenko et al. | 2016 | 63.083 | 48.728 | â | â | â | â |
| Kharchenko et al. | 2013 | 63.094 | 48.728 | â | -2.37 | -1.78 | â |
| Kharchenko et al. | 2012 | 63.094 | 48.728 | â | -2.37 | -1.78 | â |
| Froebrich et al. | 2007 | 63.087 | 48.735 | â | â | â | â |
| Dias et al. | 2002 | 63.087 | 48.735 | â | -2.37 | -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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.33 | 3.16 | 2.02 | 363 | -0.140 | 594 | â | â |
| Almeida et al. | 2025 | 2.94 | 3.11 | â | 605 | â | 314 | â | â |
| Zhang et al. | 2024 | â | â | â | â | -0.148(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 651(1) | â | â |
| Cavallo et al. | 2024 | 3.33 | 3.72 | â | 251 | 0.250 | â | â | â |
| He et al. | 2023 | 2.95 | 3.60 | â | 398 | â | â | â | â |
| Hunt & Reffert | 2023 | 2.69 | 3.21 | 2.02 | 273 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 363 | â | 594 | â | â |
| Dias et al. | 2021 | 2.94 | 3.11 | â | 605 | -0.140 | â | â | â |
| Kharchenko et al. | 2016 | 3.40 | 3.16 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.40 | 3.16 | â | 363 | â | â | â | â |
| Kharchenko et al. | 2012 | 3.40 | 3.16 | â | 363 | â | â | â | â |
| Dias et al. | 2002 | 3.40 | 3.16 | â | 363 | â | â | â | â |
(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. Silver sample.