FSR 0465
(SAI 151; MWSC 3765)
0.79
UTI
0.68
CN
1.0
Cdens
0.75
CC3
0.75
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.68 Moderately populated
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.75 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0465 is a moderately populated, very dense object of high C3 quality. Its parallax locates it at a large distance, above the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is well-studied in the literature.
Distant
High extinction
Massive
Near-solar metallicity
Old
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 357.755 | 66.187 | 0.193 | -2.559 | -0.202 | -78.906 |
| Hunt & Reffert | 2024 | 357.751 | 66.184 | 0.191 | -2.432 | -0.224 | -74.318 |
| Cavallo et al. | 2024 | 357.722 | 66.194 | 0.196 | â | â | â |
| Hunt & Reffert | 2023 | 357.751 | 66.184 | 0.191 | -2.432 | -0.224 | -74.318 |
| Just et al. | 2023 | 357.745 | 66.184 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 357.75 | 66.186 | 0.163 | -2.583 | -0.109 | â |
| Cantat-Gaudin & Anders | 2020 | 357.75 | 66.186 | 0.163 | -2.583 | -0.109 | â |
| Bica et al. | 2019 | 357.741 | 66.177 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 357.75 | 66.186 | 0.163 | -2.583 | -0.109 | â |
| Kharchenko et al. | 2016 | 357.745 | 66.184 | â | â | â | â |
| Kharchenko et al. | 2013 | 357.754 | 66.188 | â | -2.68 | -1.57 | â |
| Kharchenko et al. | 2012 | 357.754 | 66.188 | â | -3.49 | -1.56 | â |
| Glushkova et al. | 2010 | 357.727 | 66.18 | â | â | â | â |
| Froebrich et al. | 2007 | 357.742 | 66.184 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 1888* | â | â |
| Cavallo et al. | 2024 | 4.83 | 4.35 | â | 240 | -0.320 | â | â | â |
| Hunt & Reffert | 2023 | 4.11 | 3.91 | 2.15 | 1050 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1230 | â | 254 | â | â |
| Cantat-Gaudin et al. | 2020 | 6.89 | 2.33 | â | 5888 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 5.20 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 5.20 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.60 | 3.72 | â | 1230 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.60 | 3.72 | â | 1230 | â | â | â | â |
| Kharchenko et al. | 2012 | 4.60 | 3.72 | â | 1202 | â | â | â | â |
| Glushkova et al. | 2010 | 5.25 | 2.42 | â | 1585 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Bronze sample.