FSR 0498
(FoF 1321)
0.86
UTI
0.8
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
6.4 [arcmin]
- CN 0.8 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0498 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, young cluster (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | β | 7.283 | 62.398 | 0.343 | -3.279 | -0.736 | -65.659 |
| Li et al. | 2025 | 7.317 | 62.389 | 0.336 | -3.29 | -0.681 | β |
| Almeida et al. | 2025 | 7.337 | 62.39 | β | β | β | β |
| Hunt & Reffert | 2024 | 7.303 | 62.398 | 0.351 | -3.281 | -0.76 | -77.914 |
| Cavallo et al. | 2024 | 7.253 | 62.383 | 0.354 | β | β | β |
| Hunt & Reffert | 2023 | 7.303 | 62.398 | 0.351 | -3.281 | -0.76 | -77.914 |
| Almeida et al. | 2023 | 7.299 | 62.375 | β | β | β | β |
| Dias et al. | 2021 | 7.337 | 62.39 | 0.331 | -3.287 | -0.69 | β |
| Cantat-Gaudin et al. | 2020 | 7.317 | 62.389 | 0.336 | -3.29 | -0.681 | β |
| SΓ‘nchez et al. | 2020 | 7.304 | 62.416 | β | -3.137 | -0.449 | β |
| Cantat-Gaudin & Anders | 2020 | 7.317 | 62.389 | 0.336 | -3.29 | -0.681 | β |
| Liu & Pang | 2019 | 7.293 | 62.389 | 0.327 | -3.145 | -0.739 | β |
| Soubiran et al. | 2018 | 7.317 | 62.389 | β | β | β | -80.17 |
| Cantat-Gaudin et al. | 2018 | 7.317 | 62.389 | 0.336 | -3.29 | -0.681 | β |
| Dias et al. | 2014 | 7.304 | 62.416 | β | -3.62 | -0.1 | β |
| Froebrich et al. | 2007 | 7.304 | 62.416 | β | β | β | β |
| Dias et al. | 2002 | 7.304 | 62.416 | β | -3.62 | -0.1 | β |
π‘ 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 |
|---|---|---|---|---|---|---|---|---|---|
| Li et al. | 2025 | 2.43 | 1.41 | β | 97 | -0.242 | β | β | β |
| Almeida et al. | 2025 | 2.46 | 1.52 | β | 30 | β | 271 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 665* | β | β |
| Cavallo et al. | 2024 | 2.40 | 1.46 | β | 31 | -0.090 | β | β | β |
| Hunt & Reffert | 2023 | 2.54 | 1.28 | 1.37 | 64 | β | β | β | β |
| Almeida et al. | 2023 | 2.46 | 1.45 | β | 36 | -0.034 | 329* | 0.63 | β |
| Dias et al. | 2021 | 2.46 | 1.52 | β | 30 | -0.073 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 2.68 | 1.14 | β | 54 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 2.74 | β | β | β | β | β | β | β |
| Liu & Pang | 2019 | β | β | β | 7 | 0.500 | β | β | β |
| Soubiran et al. | 2018 | 2.74 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 2.74 | β | β | β | β | β | β | β |
| Dias et al. | 2002 | 1.80 | 0.46 | β | 355 | -0.340 | β | β | β |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: good fit. Silver sample.
Cavallo et al. (2024)
Gold sample.