FSR 1260
(MWSC 1235)
0.81
UTI
0.75
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
7.0 [N/pc2]
- CN 0.75 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1260 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate 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 mass 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 | 112.078 | -19.673 | 0.34 | -3.178 | 3.425 | 50.568 |
| Li et al. | 2025 | 112.088 | -19.679 | 0.321 | -3.159 | 3.444 | â |
| Almeida et al. | 2025 | 112.09 | -19.684 | â | â | â | â |
| Hunt & Reffert | 2024 | 112.081 | -19.674 | 0.341 | -3.178 | 3.435 | 39.243 |
| Cavallo et al. | 2024 | 112.07 | -19.683 | 0.342 | â | â | â |
| Hunt & Reffert | 2023 | 112.081 | -19.674 | 0.341 | -3.178 | 3.435 | 39.243 |
| Just et al. | 2023 | 112.104 | -19.678 | â | â | â | â |
| Dias et al. | 2021 | 112.09 | -19.684 | 0.315 | -3.18 | 3.425 | â |
| Cantat-Gaudin et al. | 2020 | 112.088 | -19.679 | 0.321 | -3.159 | 3.444 | â |
| Cantat-Gaudin & Anders | 2020 | 112.088 | -19.679 | 0.321 | -3.159 | 3.444 | â |
| Soubiran et al. | 2018 | 112.088 | -19.679 | â | â | â | 61.98 |
| Cantat-Gaudin et al. | 2018 | 112.088 | -19.679 | 0.321 | -3.159 | 3.444 | â |
| Kharchenko et al. | 2016 | 112.104 | -19.678 | â | â | â | â |
| Kharchenko et al. | 2013 | 112.11 | -19.68 | â | -3.43 | 6.6 | â |
| Froebrich et al. | 2007 | 112.108 | -19.689 | 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 | 2.85 | 1.17 | 1.04 | 138 | 0.055 | 247 | â | â |
| Li et al. | 2025 | 2.85 | 1.28 | â | 56 | 0.055 | â | â | â |
| Almeida et al. | 2025 | 2.69 | 1.35 | â | 82 | â | 247 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 391(1) | â | â |
| Cavallo et al. | 2024 | 3.19 | 1.37 | â | 58 | 0.180 | â | â | â |
| Hunt & Reffert | 2023 | 2.80 | 1.06 | 1.04 | 138 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 200 | â | 26 | â | â |
| Dias et al. | 2021 | 2.69 | 1.35 | â | 82 | -0.066 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.99 | 0.71 | â | 141 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.86 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.86 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.86 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.41 | 0.78 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.41 | 0.78 | â | 200 | 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: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.