FSR 1621
(MWSC 2058)
0.32
UTI
0.0
CN
0.37
Cdens
0.62
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
22
Core radius and density
1.0 [pc], 1.9 [pc-2]
- CN 0.0 Sparse
- Cdens 0.37 Loose
- CC3 0.62 Intermediate quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1621 is a sparse, loose object of intermediate 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, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is poorly studied in the literature.
(*): The parallax distance estimate (~1.49 kpc) differs significantly from the median photometric distance (~1.01 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 189.815 | -57.409 | 0.672 | -7.249 | -1.706 | -15.284 |
| Hu & Soubiran | 2025 | 189.799 | -57.417 | â | â | â | â |
| Hunt & Reffert | 2024 | 189.817 | -57.405 | 0.664 | -7.201 | -1.704 | -15.737 |
| Cavallo et al. | 2024 | 189.799 | -57.417 | 0.672 | â | â | â |
| Hunt & Reffert | 2023 | 189.817 | -57.405 | 0.664 | -7.201 | -1.704 | -15.737 |
| Just et al. | 2023 | 189.838 | -57.376 | â | â | â | â |
| Bica et al. | 2019 | 189.845 | -57.374 | â | â | â | â |
| Dib et al. | 2018 | 189.847 | -57.38 | â | â | â | â |
| Joshi et al. | 2016 | 189.847 | -57.38 | â | â | â | â |
| Kharchenko et al. | 2016 | 189.838 | -57.376 | â | â | â | â |
| Kharchenko et al. | 2013 | 189.847 | -57.38 | â | -8.57 | 2.05 | â |
| Froebrich et al. | 2007 | 189.838 | -57.376 | 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 | 1.01 | 0.63 | 0.67 | 100 | -0.040 | 50 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.270(5) | â | â | â |
| Hunt & Reffert | 2024 | 1.42 | 0.60 | 0.67 | 490 | â | 66(1) | â | â |
| Cavallo et al. | 2024 | 1.41 | 0.34 | â | 617 | 0.190 | â | â | â |
| Hunt & Reffert | 2023 | 1.42 | 0.59 | 0.67 | 490 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 100 | â | 34 | â | â |
| Dib et al. | 2018 | 1.01 | â | â | 100 | â | â | â | â |
| Joshi et al. | 2016 | 1.01 | 0.66 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.01 | 0.66 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.01 | 0.66 | â | 100 | 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.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.89 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.89 (50th percentile).