FSR 1153
(MWSC 1149)
0.78
UTI
0.52
CN
1.0
Cdens
1.0
CC3
0.7
Clit
1.0
Cdup
Stellar density (N50/rad)
10.8 [N/pc2]
- CN 0.52 Moderately populated
- Cdens 1.0 Very dense
- CC3 1.0 Very high quality
- Clit 0.7 Moderately studied
- Cdup 1.0 Unique
Overview
FSR 1153 is a moderately populated, very dense object of very high C3 quality. Its parallax locates it at a moderate distance, above the mid-plane, affected by low extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster (see Parameters). It is moderately studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 108.581 | -5.664 | 0.302 | -1.363 | 1.212 | 72.983 |
| Hunt & Reffert | 2024 | 108.588 | -5.663 | 0.283 | -1.348 | 1.197 | 72.988 |
| Cavallo et al. | 2024 | 108.565 | -5.684 | 0.282 | â | â | â |
| Hunt & Reffert | 2023 | 108.588 | -5.663 | 0.283 | -1.348 | 1.197 | 72.988 |
| Just et al. | 2023 | 108.586 | -5.658 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 108.573 | -5.658 | 0.33 | -1.376 | 1.206 | â |
| Cantat-Gaudin & Anders | 2020 | 108.573 | -5.658 | 0.33 | -1.376 | 1.206 | â |
| Bica et al. | 2019 | 108.595 | -5.672 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 108.573 | -5.658 | 0.33 | -1.376 | 1.206 | â |
| Kharchenko et al. | 2016 | 108.586 | -5.658 | â | â | â | â |
| Dias et al. | 2014 | 108.592 | -5.671 | â | -2.78 | -1.01 | â |
| Kharchenko et al. | 2013 | 108.592 | -5.66 | â | -2.4 | 0.59 | â |
| Froebrich et al. | 2007 | 108.592 | -5.671 | â | â | â | â |
| Dias et al. | 2002 | 108.592 | -5.671 | â | -2.69 | -0.9 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 3.02 | 0.45 | 1.51 | 116 | -0.420 | 393 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 277(1) | â | â |
| Cavallo et al. | 2024 | 2.47 | 0.68 | â | 55 | -0.420 | â | â | â |
| Hunt & Reffert | 2023 | 3.02 | 0.34 | 1.51 | 213 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 116 | â | 509 | â | â |
| Cantat-Gaudin & Anders | 2020 | 2.79 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 2.79 | â | â | â | â | â | â | â |
| Kharchenko et al. | 2016 | 3.10 | 0.45 | â | 116 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.10 | 0.45 | â | 116 | â | â | â | â |
| Dias et al. | 2002 | 3.10 | 0.45 | â | 116 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.