FSR 0172
(MWSC 3218)
0.81
UTI
0.77
CN
1.0
Cdens
1.0
CC3
0.65
Clit
1.0
Cdup
Radius (P>50% members)
2.6 [arcmin]
- CN 0.77 Rich
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.65 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0172 is a rich, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by high extinction. It is catalogued as a massive, near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Relatively close
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 | 300.005 | 29.219 | 0.294 | -2.526 | -6.011 | -0.742 |
| Hunt & Reffert | 2024 | 300.01 | 29.217 | 0.285 | -2.524 | -6.026 | -0.662 |
| Cavallo et al. | 2024 | 299.998 | 29.218 | 0.292 | â | â | â |
| Hunt & Reffert | 2023 | 300.01 | 29.217 | 0.285 | -2.524 | -6.026 | -0.662 |
| Just et al. | 2023 | 300.002 | 29.218 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 300.004 | 29.215 | 0.307 | -2.54 | -5.959 | â |
| Cantat-Gaudin & Anders | 2020 | 300.004 | 29.215 | 0.307 | -2.54 | -5.959 | â |
| Soubiran et al. | 2018 | 300.004 | 29.215 | â | â | â | -12.44 |
| Cantat-Gaudin et al. | 2018 | 300.004 | 29.215 | 0.307 | -2.54 | -5.959 | â |
| Kharchenko et al. | 2016 | 300.002 | 29.218 | â | â | â | â |
| Kharchenko et al. | 2013 | 300.007 | 29.221 | â | -1.79 | -4.47 | â |
| Froebrich et al. | 2007 | 300.004 | 29.224 | â | â | â | 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 |
|---|---|---|---|---|---|---|---|---|---|
| Hunt & Reffert | 2024 | â | â | â | â | â | 3101* | â | â |
| Cavallo et al. | 2024 | 3.80 | 4.85 | â | 36 | 0.410 | â | â | â |
| Hunt & Reffert | 2023 | 3.05 | 5.20 | 2.98 | 54 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1334 | â | 34 | â | â |
| Cantat-Gaudin et al. | 2020 | 3.37 | 4.10 | â | 158 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.98 | â | â | â | â | â | â | â |
| Soubiran et al. | 2018 | 2.98 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.98 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 1.69 | 2.52 | â | 1334 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.69 | 2.52 | â | 1334 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Silver sample.