THE PLACE OF THE RADCLIFFE WAVE IN THE LOCAL SYSTEM

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A review of publications devoted to the study of the characteristics of the Radcliffe wave is given. The advent of mass measurements of radial velocities of stars has recently led to a number of interesting results obtained from the analysis of spatial velocities of stars and open star clusters. An important place in the work is given to issues related to the clarification of the direct or indirect influence of magnetic fields on the process of formation of the Radcliffe wave. The hypothesis of Parker instability of the galactic magnetic field as one of the reasons for the formation of wave-type inhomogeneities in the galactic disk is discussed.

Sobre autores

V. Bobylev

Central Astronomical Observatory of the Russian Academy of Sciences, Pulkovo

Email: bob-v-vzz@rambler.ru
Russia

N. Ikhsanov

Central Astronomical Observatory of the Russian Academy of Sciences, Pulkovo

Russia

A. Bajkova

Central Astronomical Observatory of the Russian Academy of Sciences, Pulkovo

Russia

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