FSR 1421
(MWSC 1608)
0.26
UTI
0.0
CN
0.13
Cdens
0.25
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
0.6 [N/pc2]
- CN 0.0 Sparse
- Cdens 0.13 Very loose
- CC3 0.25 Low quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1421 is a sparse, very loose object of low C3 quality. Its parallax locates it at a relatively close distance, above 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 age and mass parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 134.284 | -42.506 | 0.963 | -7.115 | 4.775 | 30.713 |
| Hunt & Reffert | 2024 | 134.451 | -42.656 | 1.036 | -6.716 | 3.982 | 13.201 |
| Cavallo et al. | 2024 | 134.56 | -42.825 | 1.067 | â | â | â |
| Hunt & Reffert | 2023 | 134.451 | -42.656 | 1.036 | -6.716 | 3.982 | 13.201 |
| Just et al. | 2023 | 134.518 | -42.597 | â | â | â | â |
| He et al. | 2022 | 134.072 | -42.428 | 0.955 | -7.57 | 5.673 | â |
| Kharchenko et al. | 2016 | 134.518 | -42.597 | â | â | â | â |
| Kharchenko et al. | 2013 | 134.523 | -42.6 | â | -8.76 | 9.08 | â |
| Froebrich et al. | 2007 | 134.537 | -42.616 | 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 | 1.155 | 2.26 | 2.75 | 125 | -0.020 | 115 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 211(1) | â | â |
| Cavallo et al. | 2024 | 1.04 | 2.17 | â | 6 | -0.020 | â | â | â |
| Hunt & Reffert | 2023 | 0.90 | 2.26 | 2.75 | 7 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 200 | â | 19 | â | â |
| He et al. | 2022 | â | 2.45 | â | 50 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.27 | 2.26 | â | 200 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.27 | 2.26 | â | 200 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as optical pair (not dynamically associated) P84, along with BH_56.
Cavallo et al. (2024)
Bronze sample.