Place of the Radcliffe Wave in the Local System

Fuente: arXiv
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Main Authors: Bobylev, Vadim V., Ikhsanov, Nazar R., Bajkova, Anisa T.
Format: Preprint
Published: 2025
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author Bobylev, Vadim V.
Ikhsanov, Nazar R.
Bajkova, Anisa T.
author_facet Bobylev, Vadim V.
Ikhsanov, Nazar R.
Bajkova, Anisa T.
contents A review of publications devoted to the study of the characteristics of the Radcliffe wave has been 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 study has been 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 has been discussed.
format Preprint
id arxiv_https___arxiv_org_abs_2510_25570
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Place of the Radcliffe Wave in the Local System
Bobylev, Vadim V.
Ikhsanov, Nazar R.
Bajkova, Anisa T.
Astrophysics of Galaxies
A review of publications devoted to the study of the characteristics of the Radcliffe wave has been 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 study has been 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 has been discussed.
title Place of the Radcliffe Wave in the Local System
topic Astrophysics of Galaxies
url https://arxiv.org/abs/2510.25570