SAI 30
(MWSC 291)
Summary
SAI 30 is a poorly populated, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well above the mid-plane. It is rarely studied in the literature, with no articles listed in the last 6 years.
Warning: the low UTI value and no obvious signs of duplication (C_dup=1.0) indicates that this is quite probably an asterism, moving group, or artifact, and not a real open cluster.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 55.092 | 82.233 | – | 2.2 | 0.97 | – |
| Glushkova et al. (2010) | 55.093 | 82.233 | – | – | – | – |
| Bica et al. (2019) | 54.931 | 82.201 | – | – | – | – |
| UCC | 55.167 | 82.23 | 0.326 | -0.402 | 1.847 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.25, Dist=3100.0, Age=8.0 |
| Glushkova et al. (2010) | E(B-V)=1.25, Dist=3100.0, Age=8.0 |
Search coordinates in Bayestar19