Dolidze 37
Summary
Dolidze 37 is a sparse, very loose object of very low C3 quality. It is located at a large distance from the Sun, 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.
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) | 300.75 | 37.683 | – | -0.16 | -3.42 | – |
| Kharchenko et al. (2012) | 300.712 | 37.65 | – | -3.66 | -3.61 | – |
| Loktin & Popova (2017) | 300.72 | 37.654 | – | -3.608 | -7.549 | – |
| UCC | 300.705 | 37.65 | 0.137 | -3.748 | -5.938 | -34.165 |
Estimated members
Explore data in Colab
Fundamental parameters
| Reference | Values |
|---|---|
| Dias et al. (2002) | E(B-V)=2.311, Dist=1400.0, Age=7.585 |
| Kharchenko et al. (2012) | e_bv=2.311, distance=1400, log_age=7.585 |
| Loktin & Popova (2017) | E(B-V)=0.297, Dist=1919, logt=8.85 |
Search coordinates in Bayestar19