FSR 1460
(SAI 103; MWSC 1628)
0.62
UTI
0.76
CN
0.74
Cdens
0.75
CC3
0.42
Clit
1.0
Cdup
Nm (P>50%)
140
Core radius and density
1.5 [pc], 3.7 [pc-2]
- CN 0.76 Rich
- Cdens 0.74 Moderately dense
- CC3 0.75 High quality
- Clit 0.42 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1460 is a rich, moderately dense object of 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, metal-rich, intermediate-age cluster, but with a large variance across recent sources for the age and mass parameters (see Parameters). It is poorly studied in the literature.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 136.918 | -47.827 | 0.254 | -3.572 | 3.928 | 68.137 |
| Hunt & Reffert | 2024 | 136.908 | -47.824 | 0.256 | -3.605 | 3.946 | 24.411 |
| Cavallo et al. | 2024 | 136.921 | -47.821 | 0.287 | â | â | â |
| Hunt & Reffert | 2023 | 136.908 | -47.824 | 0.256 | -3.605 | 3.946 | 24.411 |
| Just et al. | 2023 | 136.908 | -47.822 | â | â | â | â |
| Cantat-Gaudin et al. | 2020 | 136.922 | -47.827 | 0.225 | -3.49 | 3.944 | â |
| Cantat-Gaudin & Anders | 2020 | 136.922 | -47.827 | 0.225 | -3.49 | 3.944 | â |
| Bica et al. | 2019 | 136.909 | -47.836 | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 136.922 | -47.827 | 0.225 | -3.49 | 3.944 | â |
| Dib et al. | 2018 | 136.912 | -47.825 | â | â | â | â |
| Joshi et al. | 2016 | 136.912 | -47.825 | â | â | â | â |
| Kharchenko et al. | 2016 | 136.908 | -47.822 | â | â | â | â |
| Kharchenko et al. | 2013 | 136.912 | -47.825 | â | -10.53 | 3.57 | â |
| Glushkova et al. | 2010 | 136.91 | -47.834 | â | â | â | â |
| Froebrich et al. | 2007 | 136.904 | -47.819 | 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 | 2.95 | 4.335 | 2.265 | 684 | 0.840 | 1200 | â | â |
| Hunt & Reffert | 2024 | 2.95 | 6.04 | 2.26 | 534 | â | 2334(1) | â | â |
| Cavallo et al. | 2024 | 3.55 | 5.45 | â | 135 | 0.840 | â | â | â |
| Hunt & Reffert | 2023 | 2.95 | 6.04 | 2.27 | 533 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 684 | â | 65 | â | â |
| Kounkel et al. | 2020 | 4.01 | 4.54 | â | 631 | â | â | â | â |
| Cantat-Gaudin & Anders | 2020 | 3.93 | â | â | â | â | â | â | â |
| Cantat-Gaudin et al. | 2018 | 3.93 | â | â | â | â | â | â | â |
| Dib et al. | 2018 | 1.28 | â | â | 684 | â | â | â | â |
| Joshi et al. | 2016 | 1.28 | 3.28 | â | 684 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.28 | 3.28 | â | 684 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.28 | 3.28 | â | 684 | â | â | â | â |
| Glushkova et al. | 2010 | 1.80 | 4.13 | â | 1995 | 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)
Wood sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.10 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.10 (50th percentile).