FSR 0154
(SAI 131; MWSC 3181)
0.85
UTI
0.79
CN
1.0
Cdens
0.75
CC3
0.86
Clit
1.0
Cdup
Radius (P>50% members)
2.9 [arcmin]
- CN 0.79 Rich
- Cdens 1.0 Very dense
- CC3 0.75 High quality
- Clit 0.86 Well-studied
- Cdup 1.0 Unique
Overview
FSR 0154 is a rich, very dense object of high C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age 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
Intermediate age
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | â | 297.011 | 23.354 | 0.23 | -1.635 | -4.153 | 25.55 |
| Almeida et al. | 2025 | 297.006 | 23.357 | â | â | â | â |
| Hunt & Reffert | 2024 | 297.011 | 23.353 | 0.236 | -1.648 | -4.16 | 18.557 |
| Cavallo et al. | 2024 | 297.022 | 23.364 | 0.233 | â | â | â |
| Hunt & Reffert | 2023 | 297.011 | 23.353 | 0.236 | -1.648 | -4.16 | 18.557 |
| Just et al. | 2023 | 296.99 | 23.334 | â | â | â | â |
| Dias et al. | 2021 | 297.006 | 23.357 | 0.201 | -1.597 | -4.142 | â |
| Cantat-Gaudin et al. | 2020 | 297.009 | 23.353 | 0.211 | -1.601 | -4.133 | â |
| Cantat-Gaudin & Anders | 2020 | 297.009 | 23.353 | 0.211 | -1.601 | -4.133 | â |
| Soubiran et al. | 2018 | 297.009 | 23.353 | â | â | â | 26.28 |
| Bica et al. | 2019 | 297.005 | 23.343 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 297.009 | 23.353 | 0.211 | -1.601 | -4.133 | â |
| Kharchenko et al. | 2016 | 296.99 | 23.334 | â | â | â | â |
| Kharchenko et al. | 2013 | 296.995 | 23.337 | â | -3.58 | -5.33 | â |
| Glushkova et al. | 2010 | 297.003 | 23.348 | â | â | â | â |
| Froebrich et al. | 2007 | 296.992 | 23.351 | â | â | â | â |
| Dias et al. | 2002 | 296.992 | 23.351 | â | -3.58 | -5.33 | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Almeida et al. | 2025 | 4.05 | 3.54 | â | 498 | â | 1501 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 2645* | â | â |
| Cavallo et al. | 2024 | 4.02 | 4.64 | â | 166 | -0.010 | â | â | â |
| Hunt & Reffert | 2023 | 3.85 | 4.36 | 1.67 | 221 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 10 | â | 1245 | â | â |
| Dias et al. | 2021 | 4.05 | 3.54 | â | 498 | 0.402 | â | â | â |
| Cantat-Gaudin et al. | 2020 | 3.60 | 3.52 | â | 479 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 4.17 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 4.17 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 4.17 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 4.39 | 4.68 | â | 10 | â | â | â | â |
| Kharchenko et al. | 2013 | 4.39 | 4.68 | â | 10 | â | â | â | â |
| Glushkova et al. | 2010 | 2.79 | 2.17 | â | 1122 | â | â | â | â |
| Dias et al. | 2002 | 4.39 | 4.68 | 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: invalid due to poor quality CMD. Isochrone match: worst fit.
Cavallo et al. (2024)
Gold sample.