SAI 149
(MWSC 3748)
0.71
UTI
0.38
CN
1.0
Cdens
0.62
CC3
0.78
Clit
1.0
Cdup
Stellar density (N50/rad)
9.4 [N/pc2]
- CN 0.38 Poorly populated
- Cdens 1.0 Very dense
- CC3 0.62 Intermediate quality
- Clit 0.78 Well-studied
- Cdup 1.0 Unique
Overview
SAI 149 is a poorly populated, very dense object of intermediate C3 quality. Its parallax locates it at a moderate* distance, near the mid-plane, affected by high extinction. It is catalogued as a near-solar metallicity, intermediate-age cluster, but with a large variance across recent sources for the age and metallicity parameters (see Parameters). It is well-studied in the literature.
(*): The parallax distance estimate (~3.63 kpc) differs significantly from the median photometric distance (~2.55 kpc).
Data
| Reference | Year | RA [deg] | DEC [deg] | Plx [mas] | pmRA [mas/yr] | pmDE [mas/yr] | Rv [km/s] |
|---|---|---|---|---|---|---|---|
| UCC | 99999β | 354.501 | 60.54 | 0.275 | -3.838 | -1.693 | -67.916 |
| Almeida et al. | 2025 | 354.494 | 60.562 | β | β | β | β |
| Hunt & Reffert | 2024 | 354.512 | 60.541 | 0.275 | -3.809 | -1.709 | -67.935 |
| Cavallo et al. | 2024 | 354.525 | 60.545 | 0.272 | β | β | β |
| Hunt & Reffert | 2023 | 354.512 | 60.541 | 0.275 | -3.809 | -1.709 | -67.935 |
| Dias et al. | 2021 | 354.494 | 60.562 | 0.306 | -3.903 | -1.593 | -67.324 |
| Cantat-Gaudin et al. | 2020 | 354.506 | 60.541 | 0.304 | -3.901 | -1.633 | β |
| SΓ‘nchez et al. | 2020 | 354.508 | 60.549 | β | -3.837 | -1.706 | β |
| Cantat-Gaudin & Anders | 2020 | 354.506 | 60.541 | 0.304 | -3.901 | -1.633 | β |
| Soubiran et al. | 2018 | 354.506 | 60.541 | β | β | β | -67.52 |
| Bica et al. | 2019 | 354.519 | 60.548 | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 354.506 | 60.541 | 0.304 | -3.901 | -1.633 | β |
| Loktin & Popova | 2017 | 354.51 | 60.549 | β | -1.397 | -2.203 | β |
| Dias et al. | 2014 | 354.508 | 60.549 | β | -1.57 | -2.16 | β |
| Glushkova et al. | 2010 | 354.507 | 60.549 | β | β | β | β |
| Dias et al. | 2002 | 354.508 | 60.549 | β | -1.57 | -2.16 | β |
π‘ 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 | 99999β | 2.55 | 3.44 | 1.1 | 226 | 0.317 | 284 | β | β |
| Almeida et al. | 2025 | 2.55 | 3.22 | β | 296 | β | 272 | β | β |
| Hunt & Reffert | 2024 | β | β | β | β | β | 296(1) | β | β |
| Cavallo et al. | 2024 | 2.52 | 3.66 | β | 347 | 0.490 | β | β | β |
| Hunt & Reffert | 2023 | 3.43 | 4.12 | 1.10 | 86 | β | β | β | β |
| Dias et al. | 2021 | 2.55 | 3.22 | β | 296 | 0.143 | β | β | β |
| Cantat-Gaudin et al. | 2020 | 3.42 | 2.92 | β | 282 | β | β | β | β |
| Cantat-Gaudin & Anders | 2020 | 3.00 | β | β | β | β | β | β | β |
| Soubiran et al. | 2018 | 3.00 | β | β | β | β | β | β | β |
| Cantat-Gaudin et al. | 2018 | 3.00 | β | β | β | β | β | β | β |
| Loktin & Popova | 2017 | 0.92 | 2.51 | β | 170 | β | β | β | β |
| Glushkova et al. | 2010 | 2.37 | 4.00 | β | 158 | β | β | β | β |
| Dias et al. | 2002 | 2.37 | 4.00 | β | 158 | β | β | β | β |
(N): Indicates that there are N extra values assigned to this parameter in the corresponding reference.
MOCA


Cavallo et al. (2024)
Gold sample.
Almeida et al. (2025)
Mass determination: invalid due to poor quality CMD. Isochrone match: worst fit.