SAI 90
(MWSC 1493)
0.20
UTI
0.0
CN
0.13
Cdens
0.25
CC3
0.32
Clit
1.0
Cdup
Nm (P>50%)
24
Core radius and density
1.7 [pc], 0.6 [pc-2]
- CN 0.0 Sparse
- Cdens 0.13 Very loose
- CC3 0.25 Low quality
- Clit 0.32 Poorly studied
- Cdup 1.0 Unique
Overview
SAI 90 is a sparse, very loose object of low C3 quality. Its parallax locates it at a moderate distance, below the mid-plane, affected by high extinction. It is catalogued as a very metal-rich, old cluster, but with a large variance across recent sources for the age parameter (see Parameters). It is poorly studied in the literature.
â ī¸ Warning: the low UTI value and no obvious signs of duplication (Cdup=1.0) indicate that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999â | 127.018 | -41.751 | 0.414 | -4.849 | 4.335 | â |
| Hunt & Reffert | 2024 | 127.026 | -41.754 | 0.418 | -4.822 | 4.335 | 14.297 |
| Cavallo et al. | 2024 | 126.702 | -41.79 | 0.418 | â | â | â |
| Hunt & Reffert | 2023 | 127.026 | -41.754 | 0.418 | -4.822 | 4.335 | 14.297 |
| Just et al. | 2023 | 127.018 | -41.767 | â | â | â | â |
| Bica et al. | 2019 | 126.997 | -41.767 | â | â | â | â |
| Dias et al. | 2018 | â | â | â | -4.95 | 4.24 | â |
| Sampedro et al. | 2017 | 126.996 | -41.769 | â | â | â | â |
| Kharchenko et al. | 2016 | 127.018 | -41.767 | â | â | â | â |
| Dias et al. | 2014 | 126.996 | -41.769 | â | -1.91 | 1.81 | â |
| Kharchenko et al. | 2013 | 127.023 | -41.77 | â | -3.79 | 6.32 | â |
| Glushkova et al. | 2010 | 126.995 | -41.769 | â | â | â | â |
| Dias et al. | 2002 | 126.996 | -41.769 | â | -1.91 | 1.81 | 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 | 2.74 | 3.22 | 2.69 | 1122 | 1.040 | 328 | â | â |
| Hunt & Reffert | 2024 | 2.21 | 2.72 | 2.69 | 13 | â | 248(1) | â | â |
| Cavallo et al. | 2024 | 2.56 | 2.99 | â | 38 | 1.040 | â | â | â |
| Hunt & Reffert | 2023 | 2.21 | 2.72 | 2.69 | 13 | â | â | â | â |
| Just et al. | 2023 | â | â | â | 1274 | â | 409 | â | â |
| Kharchenko et al. | 2016 | 3.11 | 3.28 | â | 1274 | â | â | â | â |
| Kharchenko et al. | 2013 | 3.11 | 3.28 | â | 1274 | â | â | â | â |
| Glushkova et al. | 2010 | 2.74 | 3.22 | â | 1122 | â | â | â | â |
| Dias et al. | 2002 | 2.74 | 3.22 | â | 1122 | â | â | â | â |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Palma et al. (2025)
Classified as tidal capture (resonant trapping pair) P7, along with CWNU_1656.
Cavallo et al. (2024)
Silver sample.
Hunt & Reffert (2024)
Classified as open cluster. CMD class: 0.05 (50th percentile).
Hunt & Reffert (2023)
Classified as open cluster. CMD class: 0.05 (50th percentile).