FSR 1149
(MWSC 1083)
0.47
UTI
0.34
CN
0.34
Cdens
0.75
CC3
0.45
Clit
1.0
Cdup
Stellar density (N50/rad)
1.7 [N/pc2]
- CN 0.34 Poorly populated
- Cdens 0.34 Loose
- CC3 0.75 High quality
- Clit 0.45 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1149 is a poorly populated, loose object of high C3 quality. Its parallax locates it at a moderate distance, near the mid-plane, affected by moderate extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the absorption parameter (see Parameters). It is poorly studied in the literature.
Note: This object shares a large percentage of members with a later reported entry. See table with shared members information.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 106.023 | -6.443 | 0.427 | -1.556 | 0.618 | 67.776 |
| Hunt & Reffert | 2024 | 106.067 | -6.446 | 0.424 | -1.536 | 0.627 | 67.778 |
| Cavallo et al. | 2024 | 106.043 | -6.438 | 0.423 | â | â | â |
| Hunt & Reffert | 2023 | 106.067 | -6.446 | 0.424 | -1.536 | 0.627 | 67.778 |
| Just et al. | 2023 | 105.991 | -6.383 | â | â | â | â |
| Bica et al. | 2019 | 106.029 | -6.4 | â | â | â | â |
| Kharchenko et al. | 2016 | 105.991 | -6.383 | â | â | â | â |
| Kharchenko et al. | 2013 | 105.997 | -6.385 | â | 1.3 | -1.63 | â |
| Froebrich et al. | 2007 | 106.025 | -6.401 | 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] | Bfrac | BSS |
|---|---|---|---|---|---|---|---|---|---|
| UCC | 99999â | 2.57 | 1.335 | 0.63 | 184 | 0.120 | 210 | â | â |
| Hunt & Reffert | 2024 | â | â | â | â | â | 158(1) | â | â |
| Cavallo et al. | 2024 | 1.85 | 0.00 | â | 141 | 0.120 | â | â | â |
| Hunt & Reffert | 2023 | 2.17 | 0.41 | 0.63 | 61 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 184 | â | 262 | â | â |
| Kharchenko et al. | 2016 | 2.97 | 2.26 | â | 184 | â | â | â | â |
| Kharchenko et al. | 2013 | 2.97 | 2.26 | â | 184 | 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.