FSR 0425
(MWSC 3710)
0.29
UTI
0.0
CN
0.06
Cdens
0.5
CC3
0.44
Clit
1.0
Cdup
Radius (P>50% members)
9.0 [arcmin]
- CN 0.0 Sparse
- Cdens 0.06 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.44 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 0425 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a very small percentage of members with at least one entry reported in the same catalogue. See table with shared members information.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Relatively close
High extinction
Low mass
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 348.557 | 61.221 | 0.348 | -4.426 | -1.856 | â |
| Just et al. | 2023 | 348.692 | 61.281 | â | â | â | â |
| Kharchenko et al. | 2016 | 348.692 | 61.281 | â | â | â | â |
| Dias et al. | 2014 | 348.658 | 61.284 | â | -0.19 | -0.93 | â |
| Kharchenko et al. | 2013 | 348.699 | 61.285 | â | -1.89 | -1.21 | â |
| Kharchenko et al. | 2012 | 348.699 | 61.285 | â | -1.89 | -1.21 | â |
| Froebrich et al. | 2007 | 348.658 | 61.284 | â | â | â | â |
| Dias et al. | 2002 | 348.658 | 61.284 | â | -0.19 | -0.93 | 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] | Bfr | BSS |
|---|---|---|---|---|---|---|---|---|---|
| Just et al. | 2023 | â | â | â | 501 | â | 36 | â | â |
| Kharchenko et al. | 2016 | 2.64 | 3.74 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.64 | 3.74 | â | 501 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.64 | 3.74 | â | 501 | â | â | â | â |
| Dias et al. | 2002 | 2.64 | 3.74 | â | 501 | â | â | â | â |
