VDBH 91
(vdBergh-Hagen 91; MWSC 1787)
Summary
VDBH 91 is a sparse, very loose object of low C3 quality. It is located at a moderate distance from the Sun, below the mid-plane. It is poorly studied in the literature, with no articles listed in the last 6 years.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 154.325 | -58.7 | – | -3.28 | 2.13 | – |
| Piskunov et al. (2008) | 154.31 | -58.693 | – | – | – | – |
| Kharchenko et al. (2012) | 154.245 | -58.695 | – | -12.1 | 2.53 | – |
| Bica et al. (2019) | 154.326 | -58.699 | – | – | – | – |
| UCC | 154.244 | -58.711 | 0.269 | -5.226 | 2.74 | 23.353 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.08, Dist=740.0, Age=8.21 |
| Piskunov et al. (2008) | E(B-V)=0.08, Dist=740, logt=8.21, logMA=1.638 |
| Kharchenko et al. (2012) | e_bv=0.083, distance=749, log_age=8.35 |
Search coordinates in Bayestar19