VDB 150
(vdBergh 150)
Summary
VDB 150 is a sparse, very loose object of very 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 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) | 333.2 | 73.333 | – | -0.57 | 9.07 | – |
| Kharchenko et al. (2012) | 333.072 | 73.37 | – | 5.32 | -3.11 | – |
| UCC | 333.142 | 73.412 | 0.305 | -3.003 | -0.539 | – |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.228, Dist=3990.0, Age=8.8 |
| Kharchenko et al. (2012) | e_bv=1.228, distance=3990, log_age=8.8 |
Search coordinates in Bayestar19