FSR 0354
(MWSC 3594)
0.45
UTI
0.7
CN
0.19
Cdens
0.38
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
5.7 [arcmin]
- CN 0.7 Moderately populated
- Cdens 0.19 Very loose
- CC3 0.38 Low quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0354 is a moderately populated, very loose object of low C3 quality. Its parallax locates it at a large* distance, above the mid-plane, affected by moderate extinction. It is catalogued as a low-mass, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~5.87 kpc) differs significantly from the median photometric distance (~1.17 kpc).
Note: This object shares a significant percentage of members with 3 later reported entries. See table with shared members information.
Relatively close
Moderate 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 | 332.755 | 57.694 | 0.17 | -2.888 | -2.03 | -48.451 |
| Just et al. | 2023 | 332.785 | 57.656 | â | â | â | â |
| Loktin & Popova | 2017 | 332.775 | 57.641 | â | -6.818 | -2.038 | â |
| Kharchenko et al. | 2016 | 332.785 | 57.656 | â | â | â | â |
| Dias et al. | 2014 | 332.8 | 57.699 | â | -0.67 | -4.0 | â |
| Kharchenko et al. | 2013 | 332.79 | 57.66 | â | -2.8 | -3.64 | â |
| Kharchenko et al. | 2012 | 332.79 | 57.66 | â | -2.8 | -3.64 | â |
| Froebrich et al. | 2007 | 332.8 | 57.699 | â | â | â | â |
| Dias et al. | 2002 | 332.8 | 57.699 | â | -0.67 | -4.0 | 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 | 100 | â | 37 | â | â |
| Loktin & Popova | 2017 | 1.88 | 1.89 | â | 178 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.17 | 1.55 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.17 | 1.55 | â | 100 | â | â | â | â |
| Kharchenko et al. | 2012 | 1.17 | 1.55 | â | 100 | â | â | â | â |
| Dias et al. | 2002 | 1.17 | 1.55 | â | 100 | â | â | â | â |
