Ruprecht 150
Summary
Ruprecht 150 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, well below the mid-plane. It is rarely studied in the literature, with no articles listed in the last 13 years.
Warning: contains less than 25 stars with P>0.5 estimated.
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) | 106.479 | -28.417 | – | -1.6 | 1.17 | – |
| Kharchenko et al. (2012) | 106.493 | -28.41 | – | -1.6 | 1.17 | – |
| UCC | 106.488 | -28.389 | 0.236 | -1.228 | 3.366 | 64.883 |
Estimated members
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Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.271, Dist=1789.0, Age=8.7 |
| Kharchenko et al. (2012) | e_bv=0.271, distance=1789, log_age=8.7 |
Search coordinates in Bayestar19