FSR 1744
(SAI 124; MWSC 2474)
0.59
UTI
0.58
CN
0.77
Cdens
1.0
CC3
0.29
Clit
1.0
Cdup
Nm (P>50%)
67
Core radius and density
1.1 [pc], 3.9 [pc-2]
- CN 0.58 Moderately populated
- Cdens 0.77 Dense
- CC3 1.0 Very high quality
- Clit 0.29 Poorly studied
- Cdup 1.0 Unique
Overview
FSR 1744 is a moderately populated, dense object of very high C3 quality. Its parallax locates it at a relatively close distance, near the mid-plane, affected by moderate extinction. It is catalogued as a metal-poor, intermediate-age cluster (see Parameters). It is poorly studied in the literature.
Note: This object shares a significant 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 | 252.958 | -42.407 | 0.59 | 0.254 | -0.137 | -2.885 |
| Hunt & Reffert | 2024 | 252.973 | -42.409 | 0.576 | 0.266 | -0.131 | -24.16 |
| Cavallo et al. | 2024 | 252.939 | -42.414 | 0.576 | â | â | â |
| Hunt & Reffert | 2023 | 252.973 | -42.409 | 0.576 | 0.266 | -0.131 | -24.16 |
| Just et al. | 2023 | 252.874 | -42.393 | â | â | â | â |
| Bica et al. | 2019 | 252.902 | -42.411 | â | â | â | â |
| Dib et al. | 2018 | 252.885 | -42.393 | â | â | â | â |
| Kharchenko et al. | 2016 | 252.874 | -42.393 | â | â | â | â |
| Kharchenko et al. | 2013 | 252.885 | -42.393 | â | -3.05 | -3.15 | â |
| Morales et al. | 2013 | 252.899 | -42.43 | â | â | â | â |
| Glushkova et al. | 2010 | 252.899 | -42.43 | â | â | â | â |
| Froebrich et al. | 2007 | 252.9 | -42.415 | 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 | 1.84 | 2.615 | 2.29 | 398 | -0.730 | 252 | â | â |
| Hunt & Reffert | 2024 | 1.59 | 1.83 | 2.29 | 163 | â | 450(1) | â | â |
| Cavallo et al. | 2024 | 2.49 | 2.08 | â | 324 | -0.730 | â | â | â |
| Hunt & Reffert | 2023 | 1.60 | 1.83 | 2.29 | 163 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 398 | â | 54 | â | â |
| Dib et al. | 2018 | 1.84 | â | â | 398 | â | â | â | â |
| Kharchenko et al. | 2016 | 1.84 | 3.15 | â | 398 | â | â | â | â |
| Kharchenko et al. | 2013 | 1.84 | 3.15 | â | 398 | â | â | â | â |
| Morales et al. | 2013 | 3.13 | â | â | 708 | â | â | â | â |
| Glushkova et al. | 2010 | 3.13 | 8.14 | â | 708 | 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)
Bronze sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.83 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.83 (50th percentile).
Morales et al. (2013)
Classified as morphological type 'OC2' (totally exposed cluster without correlation with ATLASGAL emission). Morphological flag: exposed cluster, without submm emission.