FSR 0460
(SAI 153; MWSC 3783)
0.82
UTI
0.77
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
2.1 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0460 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is well-studied in the literature.
Very distant
High extinction
Massive
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 | 359.768 | 60.693 | 0.154 | -1.348 | -0.306 | -72.018 |
| Hu & Soubiran | 2025 | 359.767 | 60.698 | â | â | â | â |
| Hunt & Reffert | 2024 | 359.762 | 60.691 | 0.154 | -1.351 | -0.305 | -71.433 |
| Cavallo et al. | 2024 | 359.767 | 60.698 | 0.149 | â | â | â |
| He et al. | 2023 | 359.772 | 60.693 | 0.153 | -1.346 | -0.309 | -72.02 |
| Hunt & Reffert | 2023 | 359.762 | 60.691 | 0.154 | -1.351 | -0.305 | -71.433 |
| Just et al. | 2023 | 359.763 | 60.69 | â | â | â | â |
| Bica et al. | 2019 | 359.788 | 60.674 | â | â | â | â |
| Kharchenko et al. | 2016 | 359.763 | 60.69 | â | â | â | â |
| Dias et al. | 2014 | 359.792 | 60.692 | â | -1.51 | -0.25 | â |
| Kharchenko et al. | 2013 | 359.772 | 60.694 | â | 1.71 | -3.26 | â |
| Kharchenko et al. | 2012 | 359.772 | 60.694 | â | 1.71 | -3.26 | â |
| Glushkova et al. | 2010 | 359.779 | 60.678 | â | â | â | â |
| Froebrich et al. | 2007 | 359.792 | 60.692 | â | â | â | â |
| Dias et al. | 2002 | 359.792 | 60.692 | â | -1.51 | -0.25 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hu & Soubiran | 2025 | â | â | â | â | -0.360* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2601* | â | â |
| Cavallo et al. | 2024 | 4.99 | 3.16 | â | 1148 | -0.220 | â | â | â |
| He et al. | 2023 | 4.37 | 3.00 | â | 1585 | â | â | â | â |
| Hunt & Reffert | 2023 | 5.31 | 3.31 | 1.61 | 857 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 507 | â | 817 | â | â |
| Kharchenko et al. | 2016 | 5.88 | 3.42 | â | 507 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.88 | 3.42 | â | 507 | â | â | â | â |
| Kharchenko et al. | 2012 | 5.88 | 3.42 | â | 507 | â | â | â | â |
| Glushkova et al. | 2010 | 4.90 | 2.67 | â | 1585 | â | â | â | â |
| Dias et al. | 2002 | 5.88 | 3.42 | â | 507 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.