FSR 0634
(SAI 29; MWSC 292)
0.65
UTI
0.76
CN
1.0
Cdens
0.5
CC3
0.5
Clit
1.0
Cdup
Radius (P>50% members)
2.2 [arcmin]
- CN 0.76 Rich
- Cdens 1.0 Very dense
- CC3 0.5 Intermediate quality
- Clit 0.5 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 0634 is a rich, very dense object of intermediate C3 quality. Its parallax locates it at a moderate distance, above 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 | 55.088 | 59.421 | 0.271 | 1.018 | -0.44 | -22.338 |
| Hunt & Reffert | 2024 | 55.087 | 59.417 | 0.278 | 1.003 | -0.452 | -22.337 |
| Cavallo et al. | 2024 | 55.099 | 59.411 | 0.271 | â | â | â |
| He et al. | 2023 | 55.084 | 59.422 | 0.28 | 1.015 | -0.433 | -22.34 |
| Hunt & Reffert | 2023 | 55.087 | 59.417 | 0.278 | 1.003 | -0.452 | -22.337 |
| Bica et al. | 2019 | 55.11 | 59.418 | â | â | â | â |
| Glushkova et al. | 2010 | 55.09 | 59.414 | â | â | â | â |
| Froebrich et al. | 2007 | 55.1 | 59.419 | â | â | â | â |
| Dias et al. | 2002 | 55.1 | 59.419 | â | 26.81 | -20.15 | 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 | 1271* | â | â |
| Cavallo et al. | 2024 | 4.21 | 3.49 | â | 269 | 0.300 | â | â | â |
| He et al. | 2023 | 2.88 | 3.30 | â | 501 | â | â | â | â |
| Hunt & Reffert | 2023 | 3.16 | 3.22 | 2.25 | 236 | â | â | â | â |
| Glushkova et al. | 2010 | 2.80 | 2.60 | â | 1000 | â | â | â | â |
| Dias et al. | 2002 | 2.30 | 3.56 | â | 895 | â | â | â | â |
(*): Indicates that this parameter is assigned more than one value in the corresponding reference.


Cavallo et al. (2024)
Gold sample.