FSR 0394
(SAI 147; MWSC 3675)
0.81
UTI
0.78
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Stellar density (N50/rad)
22.2 [N/pc2]
- CN 0.78 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0394 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is well-studied in the literature.
Note: This object shares a small 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 | 343.798 | 58.714 | 0.244 | -3.722 | -1.28 | -69.871 |
| Hu & Soubiran | 2025 | 343.774 | 58.718 | â | â | â | â |
| Hunt & Reffert | 2024 | 343.813 | 58.711 | 0.249 | -3.732 | -1.301 | -70.836 |
| Cavallo et al. | 2024 | 343.774 | 58.718 | 0.233 | â | â | â |
| Hunt & Reffert | 2023 | 343.813 | 58.711 | 0.249 | -3.732 | -1.301 | -70.836 |
| Just et al. | 2023 | 343.777 | 58.721 | â | â | â | â |
| Donor et al. | 2020 | 343.785 | 58.725 | â | -3.84 | -1.2 | -70.3 |
| Bica et al. | 2019 | 343.773 | 58.719 | â | â | â | â |
| Kharchenko et al. | 2016 | 343.777 | 58.721 | â | â | â | â |
| Kharchenko et al. | 2013 | 343.785 | 58.725 | â | -5.62 | 1.78 | â |
| Kharchenko et al. | 2012 | 343.785 | 58.725 | â | -5.62 | 1.78 | â |
| Glushkova et al. | 2010 | 343.77 | 58.715 | â | â | â | â |
| Froebrich et al. | 2007 | 343.783 | 58.725 | â | â | â | â |
| Dias et al. | 2002 | 343.783 | 58.725 | â | -5.62 | 1.78 | 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 | 4.74 | 3.1 | 2.33 | 1585 | -0.150 | 1558 | â | â |
| Hu & Soubiran | 2025 | â | â | â | â | -0.400(5) | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2051(1) | â | â |
| Cavallo et al. | 2024 | 5.50 | 3.34 | â | 977 | -0.150 | â | â | â |
| Hunt & Reffert | 2023 | 3.68 | 3.16 | 2.33 | 1671 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1585 | â | 1064 | â | â |
| Donor et al. | 2020 | â | â | â | â | -0.100 | â | â | â |
| Kharchenko et al. | 2016 | 4.74 | 3.10 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.74 | 3.10 | â | 1585 | â | â | â | â |
| Kharchenko et al. | 2012 | 4.74 | 3.10 | â | 1585 | â | â | â | â |
| Glushkova et al. | 2010 | 5.57 | 2.17 | â | 2512 | â | â | â | â |
| Dias et al. | 2002 | 4.74 | 3.10 | â | 1585 | 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.