FSR 1441
(MWSC 1524)
0.78
UTI
0.58
CN
1.0
Cdens
0.75
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
16.7 [N/pc2]
- CN 0.58 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1441 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below 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 | 129.88 | -47.1 | 0.203 | -3.677 | 3.602 | 58.654 |
| Li et al. | 2025 | 129.88 | -47.098 | 0.189 | -3.723 | 3.567 | â |
| Hu & Soubiran | 2025 | 129.874 | -47.099 | â | â | â | â |
| Hunt & Reffert | 2024 | 129.885 | -47.096 | 0.21 | -3.683 | 3.611 | 57.565 |
| Cavallo et al. | 2024 | 129.874 | -47.099 | 0.211 | â | â | â |
| Hunt & Reffert | 2023 | 129.885 | -47.096 | 0.21 | -3.683 | 3.611 | 57.565 |
| Just et al. | 2023 | 129.865 | -47.097 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 129.88 | -47.098 | 0.189 | -3.723 | 3.567 | â |
| Cantat-Gaudin & Anders | 2020 | 129.88 | -47.098 | 0.189 | -3.723 | 3.567 | â |
| Soubiran et al. | 2018 | 129.88 | -47.098 | â | â | â | 124.82 |
| Cantat-Gaudin et al. | 2018 | 129.88 | -47.098 | 0.189 | -3.723 | 3.567 | â |
| Kharchenko et al. | 2016 | 129.865 | -47.097 | â | â | â | â |
| Dias et al. | 2014 | 129.9 | -47.108 | â | -1.13 | 3.46 | â |
| Kharchenko et al. | 2013 | 129.87 | -47.1 | â | -5.05 | 7.73 | â |
| Froebrich et al. | 2007 | 129.9 | -47.108 | â | â | â | â |
| Dias et al. | 2002 | 129.9 | -47.108 | â | -1.13 | 3.46 | 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 | 4.325 | 1.94 | 1.95 | 537 | -0.050 | 407 | â | â |
| Li et al. | 2025 | 4.56 | 2.02 | â | 537 | -0.015 | â | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.130(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 756(1) | â | â |
| Cavallo et al. | 2024 | 3.37 | 2.15 | â | 661 | -0.050 | â | â | â |
| Hunt & Reffert | 2023 | 4.30 | 2.03 | 1.95 | 593 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 537 | â | 58 | â | â |
| Cantat-Gaudin et al. | 2020 | 4.35 | 1.39 | â | 708 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.58 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.58 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.58 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.66 | 1.94 | â | 537 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.66 | 1.94 | â | 537 | â | â | â | â |
| Dias et al. | 2002 | 1.66 | 1.94 | â | 537 | 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.