FSR 0320
(MWSC 3530)
0.72
UTI
0.55
CN
1.0
Cdens
0.75
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
3.9 [arcmin]
- CN 0.55 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0320 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a moderate* distance, above the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the metallicity parameter (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~2.20 kpc) differs significantly from the median photometric distance (~4.72 kpc).
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Distant
High extinction
Near-solar metallicity
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 323.844 | 53.655 | 0.454 | -2.538 | -2.848 | -17.258 |
| Zhang et al. | 2024 | 323.84 | 53.662 | â | â | â | â |
| Hunt & Reffert | 2024 | 323.84 | 53.662 | 0.439 | -2.535 | -2.83 | -12.664 |
| Cavallo et al. | 2024 | 323.843 | 53.646 | 0.455 | â | â | â |
| Hunt & Reffert | 2023 | 323.84 | 53.662 | 0.439 | -2.535 | -2.83 | -12.664 |
| Just et al. | 2023 | 323.845 | 53.697 | â | â | â | â |
| Kharchenko et al. | 2016 | 323.845 | 53.697 | â | â | â | â |
| Dias et al. | 2014 | 323.858 | 53.686 | â | -0.94 | 0.83 | â |
| Kharchenko et al. | 2013 | 323.85 | 53.7 | â | -4.55 | -1.63 | â |
| Kharchenko et al. | 2012 | 323.85 | 53.7 | â | -4.55 | -1.63 | â |
| Froebrich et al. | 2007 | 323.858 | 53.686 | â | â | â | â |
| Dias et al. | 2002 | 323.858 | 53.686 | â | -1.28 | 0.35 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Zhang et al. | 2024 | â | â | â | â | -0.139* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 202* | â | â |
| Cavallo et al. | 2024 | 1.91 | 1.70 | â | 170 | 0.200 | â | â | â |
| Hunt & Reffert | 2023 | 2.07 | 1.75 | 0.52 | 57 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 708 | â | 562 | â | â |
| Kharchenko et al. | 2016 | 4.72 | 3.16 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.72 | 3.16 | â | 708 | â | â | â | â |
| Kharchenko et al. | 2012 | 4.72 | 3.16 | â | 708 | â | â | â | â |
| Dias et al. | 2002 | 4.72 | 3.16 | â | 708 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.