FSR 0756
(MWSC 375)
0.35
UTI
0.0
CN
0.16
Cdens
0.5
CC3
0.55
Clit
1.0
Cdup
Radius (P>50% members)
4.7 [arcmin]
- CN 0.0 Sparse
- Cdens 0.16 Very loose
- CC3 0.5 Intermediate quality
- Clit 0.55 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0756 is a sparse, very loose object of intermediate C3 quality. Its parallax locates it at a moderate* distance, well below the mid-plane, affected by moderate extinction. It is catalogued as an intermediate-age cluster (see Parameters). It is moderately studied in the literature.
(*): The parallax distance estimate (~3.87 kpc) differs significantly from the median photometric distance (~2.17 kpc).
Relatively close
Moderate extinction
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 66.038 | 29.712 | 0.259 | 0.421 | 0.01 | â |
| Just et al. | 2023 | 66.045 | 29.714 | â | â | â | â |
| Bica et al. | 2019 | 66.065 | 29.724 | â | â | â | â |
| Loktin & Popova | 2017 | 66.06 | 29.729 | â | 0.428 | -5.558 | â |
| Kharchenko et al. | 2016 | 66.045 | 29.714 | â | â | â | â |
| Dias et al. | 2014 | 66.054 | 29.704 | â | 1.78 | -2.72 | â |
| Kharchenko et al. | 2013 | 66.054 | 29.715 | â | 1.1 | -4.45 | â |
| Kharchenko et al. | 2012 | 66.054 | 29.71 | â | -1.7 | -3.95 | â |
| Froebrich et al. | 2007 | 66.067 | 29.725 | â | â | â | â |
| Dias et al. | 2002 | 66.054 | 29.704 | â | 1.78 | -2.72 | 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 | 624 | â | 267 | â | â |
| Loktin & Popova | 2017 | 2.14 | 0.79 | â | 933 | â | â | â | â |
| Kharchenko et al. | 2016 | 2.70 | 2.33 | â | 624 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.70 | 2.33 | â | 624 | â | â | â | â |
| Kharchenko et al. | 2012 | 2.17 | 2.85 | â | 7 | â | â | â | â |
| Dias et al. | 2002 | 1.80 | 3.01 | â | 302 | â | â | â | â |
