FSR 0198
(SAI 134; MWSC 3232; MWSC 3230)
0.85
UTI
0.76
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
3.5 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0198 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, very young cluster (see Parameters). It is well-studied in the literature.
Relatively close
Moderate extinction
Near-solar metallicity
Very young
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 300.611 | 35.685 | 0.472 | -3.523 | -6.57 | â |
| Almeida et al. | 2025 | 300.615 | 35.67 | â | â | â | â |
| Celli et al. | 2024 | 300.614 | 35.681 | â | â | â | â |
| Almeida et al. | 2023 | 300.603 | 35.673 | â | â | â | â |
| Just et al. | 2023 | 300.613 | 35.682 | â | â | â | â |
| Dias et al. | 2021 | 300.615 | 35.67 | 0.489 | -3.622 | -6.643 | â |
| Cantat-Gaudin et al. | 2020 | 300.614 | 35.681 | 0.486 | -3.56 | -6.611 | â |
| Cantat-Gaudin & Anders | 2020 | 300.614 | 35.681 | 0.486 | -3.56 | -6.611 | â |
| Soubiran et al. | 2018 | 300.614 | 35.681 | â | â | â | 12.13 |
| Bica et al. | 2019 | 300.608 | 35.694 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 300.614 | 35.681 | 0.486 | -3.56 | -6.611 | â |
| Kharchenko et al. | 2016 | 300.613 | 35.682 | â | â | â | â |
| Dias et al. | 2014 | 300.6 | 35.693 | â | -3.71 | -3.74 | -13.0 |
| Kharchenko et al. | 2013 | 300.618 | 35.685 | â | -3.34 | -3.0 | 11.0 |
| Glushkova et al. | 2010 | 300.612 | 35.676 | â | â | â | â |
| Froebrich et al. | 2007 | 300.6 | 35.689 | â | â | â | â |
| Dias et al. | 2002 | 300.613 | 35.675 | â | -2.63 | -4.93 | -13.0 |
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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 1.83 | 2.58 | â | 9 | â | 576 | â | â |
| Celli et al. | 2024 | â | â | â | 5 | â | 451 | â | â |
| Almeida et al. | 2023 | 1.84 | 2.90 | â | 7 | 0.103 | 545* | 0.68 | â |
| Just et al. | 2023 | â | â | â | 4 | â | 404 | â | â |
| Dias et al. | 2021 | 1.83 | 2.58 | â | 9 | 0.209 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 2.18 | 2.49 | â | 5 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 1.94 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 1.94 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 1.94 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 2.30 | 2.77 | â | 4 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.30 | 2.77 | â | 4 | â | â | â | â |
| Dias et al. | 2002 | 1.70 | 2.98 | â | 10 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Almeida et al. (2025)
Mass determination: intermediate fit. Isochrone match: intermediate fit.