Dolidze 38
Summary
Dolidze 38 is a poorly populated, very loose object of low C3 quality. It is located at a large distance from the Sun, well above the mid-plane. It is poorly studied in the literature, with no articles listed in the last 8 years.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 301.425 | 41.2 | – | -1.73 | -6.11 | – |
| Piskunov et al. (2008) | 301.389 | 41.196 | – | – | – | – |
| Kharchenko et al. (2012) | 301.47 | 41.195 | – | -2.82 | -1.41 | – |
| Loktin & Popova (2017) | 301.425 | 41.2 | – | -0.675 | -0.348 | – |
| UCC | 301.484 | 41.177 | 0.126 | -3.016 | -3.466 | -28.186 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.15, Dist=1200.0, Age=8.95 |
| Piskunov et al. (2008) | E(B-V)=0.15, Dist=1200, logt=8.95, logMA=2.481 |
| Kharchenko et al. (2012) | e_bv=0.229, distance=1532, log_age=9.165 |
| Loktin & Popova (2017) | E(B-V)=0.232, Dist=3295, logt=9.35 |
Search coordinates in Bayestar19