FSR 0278
(Teutsch J2031.0+5102; MWSC 3355; FoF 2199)
0.89
UTI
0.76
CN
1.0
Cdens
1.0
CC3
0.84
Clit
1.0
Cdup
Stellar density (N50/rad)
16.2 [N/pc2]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.84 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0278 is a rich, very dense object of very high C3 quality. Its parallax locates it at a relatively close distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, old cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is well-studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 307.754 | 51.02 | 0.575 | -4.599 | -9.759 | -9.206 |
| Li et al. | 2025 | 307.761 | 51.021 | 0.554 | -4.615 | -9.738 | â |
| Hu & Soubiran | 2025 | 307.754 | 51.016 | â | â | â | â |
| Almeida et al. | 2025 | 307.761 | 51.023 | â | â | â | â |
| Zhang et al. | 2024 | 307.762 | 51.017 | â | â | â | â |
| Hunt & Reffert | 2024 | 307.762 | 51.017 | 0.578 | -4.602 | -9.737 | -13.142 |
| Cavallo et al. | 2024 | 307.754 | 51.016 | 0.578 | â | â | â |
| Hunt & Reffert | 2023 | 307.762 | 51.017 | 0.578 | -4.602 | -9.737 | -13.142 |
| Almeida et al. | 2023 | 307.768 | 51.025 | â | â | â | â |
| Dias et al. | 2021 | 307.761 | 51.023 | 0.556 | -4.597 | -9.738 | -6.942 |
| Cantat-Gaudin et al. | 2020 | 307.761 | 51.021 | 0.554 | -4.615 | -9.738 | â |
| Cantat-Gaudin & Anders | 2020 | 307.761 | 51.021 | 0.554 | -4.615 | -9.738 | â |
| Liu & Pang | 2019 | 307.742 | 51.002 | 0.574 | -4.64 | -9.747 | â |
| Soubiran et al. | 2018 | 307.761 | 51.021 | â | â | â | -7.94 |
| Bica et al. | 2019 | 307.767 | 51.044 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 307.761 | 51.021 | 0.554 | -4.615 | -9.738 | â |
| Froebrich et al. | 2007 | 307.738 | 51.035 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 1.7 | 0.86 | 1.61 | 2290 | -0.017 | 356 | 0.78 | â |
| Li et al. | 2025 | 1.69 | 0.86 | â | 2391 | -0.037 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.090(5) | â | â | â |
| Almeida et al. | 2025 | 1.60 | 1.03 | â | 2466 | â | 210 | â | â |
| Zhang et al. | 2024 | â | â | â | â | 0.053(1) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 356(1) | â | â |
| Cavallo et al. | 2024 | 1.72 | 0.78 | â | 1738 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.67 | 1.06 | 1.61 | 767 | â | â | â | â |
| Almeida et al. | 2023 | 1.67 | 0.86 | â | 2529 | -0.017 | 542(1) | 0.78 | â |
| Dias et al. | 2021 | 1.60 | 1.03 | â | 2466 | -0.125 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 1.71 | 0.85 | â | 2188 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.71 | â | â | â | â | â | â | â |
| Liu & Pang | 2019 | â | â | â | 1100 | 0.500 | â | â | â |
| Soubiran et al. | 2018 | 1.71 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.71 | â | â | â | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


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