FSR 0480
(SAI 3; MWSC 25)
0.83
UTI
0.82
CN
1.0
Cdens
0.75
CC3
0.79
Clit
1.0
Cdup
Radius (P>50% members)
3.4 [arcmin]
- CN 0.82 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.79 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0480 is a rich, very dense object of high C3 quality. Its parallax locates it at a large distance, below the mid-plane, affected by moderate extinction. It is catalogued as a massive, near-solar metallicity, old cluster (see Parameters). It is well-studied in the literature.
Very distant
Moderate 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 | 3.726 | 61.491 | 0.178 | -2.772 | -0.345 | -52.534 |
| Hu & Soubiran | 2025 | 3.72 | 61.507 | â | â | â | â |
| Hunt & Reffert | 2024 | 3.775 | 61.509 | 0.165 | -2.772 | -0.342 | -52.136 |
| Cavallo et al. | 2024 | 3.72 | 61.507 | 0.169 | â | â | â |
| He et al. | 2023 | 3.722 | 61.492 | 0.169 | -2.779 | -0.344 | -52.56 |
| Hunt & Reffert | 2023 | 3.775 | 61.509 | 0.165 | -2.772 | -0.342 | -52.136 |
| Just et al. | 2023 | 3.727 | 61.468 | â | â | â | â |
| Bica et al. | 2019 | 3.719 | 61.472 | â | â | â | â |
| Kharchenko et al. | 2016 | 3.727 | 61.468 | â | â | â | â |
| Dias et al. | 2014 | 3.729 | 61.473 | â | -1.72 | -1.82 | â |
| Kharchenko et al. | 2013 | 3.736 | 61.471 | â | -0.31 | -2.33 | â |
| Kharchenko et al. | 2012 | 3.736 | 61.471 | â | -0.14 | -1.97 | â |
| Glushkova et al. | 2010 | 3.707 | 61.477 | â | â | â | â |
| Froebrich et al. | 2007 | 3.729 | 61.473 | â | â | â | â |
| Dias et al. | 2002 | 3.729 | 61.473 | â | -1.66 | -1.81 | 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 | -0.410* | â | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 3063* | â | â |
| Cavallo et al. | 2024 | 6.37 | 2.84 | â | 2089 | -0.500 | â | â | â |
| He et al. | 2023 | 5.01 | 3.10 | â | 1585 | â | â | â | â |
| Hunt & Reffert | 2023 | 4.90 | 3.21 | 2.19 | 668 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1995 | â | 1849 | â | â |
| Kharchenko et al. | 2016 | 5.49 | 2.90 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2013 | 5.49 | 2.90 | â | 1995 | â | â | â | â |
| Kharchenko et al. | 2012 | 5.49 | 2.90 | â | 1995 | â | â | â | â |
| Glushkova et al. | 2010 | 6.90 | 2.11 | â | 1585 | â | â | â | â |
| Dias et al. | 2002 | 5.49 | 2.90 | â | 1995 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.