TY - CHAP

T1 - The Local Stellar system: kinematics derived from the HIPPARCOS catalogue.

AU - Tsvetkov, A.S.

PY - 1997

Y1 - 1997

N2 - 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.

AB - 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.

KW - Local Stellar System

KW - Hipparcos

KW - Galaxy rotation

M3 - статья в сборнике

SP - 1

EP - 4

BT - Jornees 1997, Systemes de reference spatio-temporels

ER -