FSR 1411
(MWSC 1505)
0.35
UTI
0.0
CN
0.5
Cdens
0.75
CC3
0.26
Clit
1.0
Cdup
Nm (P>50%)
21
Core radius and density
0.9 [pc], 2.5 [pc-2]
- CN 0.0 Sparse
- Cdens 0.5 Moderately dense
- CC3 0.75 High quality
- Clit 0.26 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1411 is a sparse, moderately 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, young cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~2.03 kpc) differs significantly from the median photometric distance (~1.41 kpc).
Note: This object shares a large percentage of members with a later reported entry. 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 | 128.66 | -43.946 | 0.492 | -5.639 | 5.271 | â |
| Hunt & Reffert | 2024 | 128.674 | -43.954 | 0.496 | -5.639 | 5.301 | â |
| Cavallo et al. | 2024 | 128.69 | -43.924 | 0.497 | â | â | â |
| Hunt & Reffert | 2023 | 128.674 | -43.954 | 0.496 | -5.639 | 5.301 | â |
| Just et al. | 2023 | 128.59 | -43.857 | â | â | â | â |
| Dib et al. | 2018 | 128.595 | -43.86 | â | â | â | â |
| Joshi et al. | 2016 | 128.595 | -43.86 | â | â | â | â |
| Kharchenko et al. | 2016 | 128.59 | -43.857 | â | â | â | â |
| Kharchenko et al. | 2013 | 128.595 | -43.86 | â | -3.67 | 2.37 | â |
| Froebrich et al. | 2007 | 128.608 | -43.848 | 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 | 1.405 | 1.97 | 1.56 | 32 | -0.300 | 113 | â | â |
| Liu et al. | 2025 | 4.61 | 0.81 | â | 18 | â | â | â | â |
| Hunt & Reffert | 2024 | 1.90 | 2.42 | 1.56 | 37 | â | 151(1) | â | â |
| Cavallo et al. | 2024 | 1.91 | 2.82 | â | 58 | -0.300 | â | â | â |
| Hunt & Reffert | 2023 | 1.90 | 2.42 | 1.56 | 37 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 32 | â | 75 | â | â |
| Dib et al. | 2018 | 0.91 | â | â | 32 | â | â | â | â |
| Joshi et al. | 2016 | 0.91 | 1.97 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2016 | 0.91 | 1.97 | â | 32 | â | â | â | â |
| Kharchenko et al. | 2013 | 0.91 | 1.97 | â | 32 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Liu et al. (2025)
Classified as primordial binary cluster 149 along with UBC_1585.
Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P20, along with UBC_1585.
Cavallo et al. (2024)
Gold sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.90 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.90 (50th percentile).