The rotational parameters of the Local Stellar system are derived from the proper motions of the HIPPARCOS catalogue. The hypothesis that the one of the phenomenon of the Local Stellar system is the Gould’s Belt is adopted. Rotation of stars of different spectral types is investigated. The most likely geometrical and kinematical descriptions of the Local Stellar system are made. The solutions derived on the matherial of GC reduced onto various fundamental systems and the PPM catalogue are considered.
|Язык оригинала||не определен|
|Название основной публикации||Jornees 1997, Systemes de reference spatio-temporels|
|Состояние||Опубликовано - 1997|