VDBH 214
(vdBergh-Hagen 214)
Summary
VDBH 214 is a sparse, very loose object of very low C3 quality. It is located at a moderate distance from the Sun, 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) | 256.425 | -36.667 | – | -4.88 | -1.56 | – |
| Kharchenko et al. (2012) | 256.418 | -36.667 | – | -2.99 | -6.5 | – |
| UCC | 256.469 | -36.657 | 0.264 | -4.461 | -2.76 | -63.527 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=1.301, Dist=1723.0, Age=7.7 |
| Kharchenko et al. (2012) | e_bv=0.645, distance=1579, log_age=8.71 |
Search coordinates in Bayestar19