FSR 1378
(SAI 85; MWSC 1412)
0.82
UTI
0.87
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
33.0 [N/pc2]
- CN 0.87 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 1378 is a rich, very dense object of high C3 quality. Its parallax locates it at a relatively close 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 age, metallicity, and mass parameters (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 | 120.3 | -40.676 | 0.606 | -5.685 | 11.945 | 27.343 |
| Hu & Soubiran | 2025 | 120.31 | -40.676 | â | â | â | â |
| Hunt & Reffert | 2024 | 120.311 | -40.681 | 0.608 | -5.683 | 11.94 | 28.111 |
| Cavallo et al. | 2024 | 120.31 | -40.676 | 0.608 | â | â | â |
| Hunt & Reffert | 2023 | 120.311 | -40.681 | 0.608 | -5.683 | 11.94 | 28.111 |
| Just et al. | 2023 | 120.325 | -40.672 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 120.304 | -40.676 | 0.588 | -5.659 | 11.934 | â |
| Cantat-Gaudin & Anders | 2020 | 120.304 | -40.676 | 0.588 | -5.659 | 11.934 | â |
| Soubiran et al. | 2018 | 120.304 | -40.676 | â | â | â | 26.03 |
| Bica et al. | 2019 | 120.294 | -40.677 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 120.304 | -40.676 | 0.588 | -5.659 | 11.934 | â |
| Kharchenko et al. | 2016 | 120.325 | -40.672 | â | â | â | â |
| Kharchenko et al. | 2013 | 120.328 | -40.675 | â | -8.02 | 9.11 | â |
| Glushkova et al. | 2010 | 120.298 | -40.678 | â | â | â | â |
| Froebrich et al. | 2007 | 120.329 | -40.684 | 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 | 1.62 | 2.26 | 2.28 | 631 | 0.095 | 952 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.100(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 1706(1) | â | â |
| Cavallo et al. | 2024 | 1.69 | 1.75 | â | 1698 | 0.290 | â | â | â |
| Hunt & Reffert | 2023 | 1.56 | 1.81 | 2.28 | 1072 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 100 | â | 197 | â | â |
| Cantat-Gaudin et al. | 2020 | 1.58 | 1.11 | â | 2239 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.62 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.62 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.62 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.56 | 2.71 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.56 | 2.71 | â | 100 | â | â | â | â |
| Glushkova et al. | 2010 | 2.23 | 3.75 | â | 631 | 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.