Dolidze 36
Summary
Dolidze 36 is a sparse, very loose object of very 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.
Warning: contains less than 25 stars with P>0.5 estimated.
Positions
| Reference | RA | DEC | Plx | pmRA | pmDE | Rv |
|---|---|---|---|---|---|---|
| Dias et al. (2002) | 300.625 | 42.1 | – | -1.47 | -3.39 | 77.0 |
| Piskunov et al. (2008) | 300.591 | 42.151 | – | – | – | – |
| Kharchenko et al. (2012) | 300.615 | 42.165 | – | 0.7 | -2.44 | – |
| Loktin & Popova (2017) | 300.54 | 42.014 | – | -0.93 | -4.477 | 77.0 |
| UCC | 300.58 | 42.098 | 0.171 | -3.359 | -4.088 | -37.194 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=0.22, Dist=900.0, Age=8.83 |
| Piskunov et al. (2008) | E(B-V)=0.22, Dist=900, logt=8.83, logMA=2.072 |
| Kharchenko et al. (2012) | e_bv=0.208, distance=970, log_age=8.92 |
| Loktin & Popova (2017) | E(B-V)=0.036, Dist=2160, logt=9.8 |
Search coordinates in Bayestar19