Place of the Radcliffe Wave in the Local System

Abstract

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.

18 page, 6 figures

References in corpus (37)

• Gaia Data Release 3: Summary of the content and survey properties
• Trigonometric Parallaxes of Massive Star Forming Regions: VI. Galactic Structure, Fundamental Parameters and Non-Circular Motions
• Trigonometric Parallaxes Of High-Mass Star Forming Regions: Our View Of The Milky Way
• Painting a portrait of the Galactic disc with its stellar clusters
• Gaia-2MASS 3D maps of Galactic interstellar dust within 3 kpc
• Improving the open cluster census. II. An all-sky cluster catalogue with Gaia DR3
• A Large Catalog of Accurate Distances to Local Molecular Clouds: The Gaia DR2 Edition
• A Compendium of Distances to Molecular Clouds in the Star Formation Handbook
• Updated Gaia-2MASS 3D maps of Galactic interstellar dust
• A Galactic-scale gas wave in the Solar Neighborhood
• A parsec-scale Galactic 3D dust map out to 1.25 kpc from the Sun
• Identification of Young Stellar Object candidates in the $Gaia$ DR2 x AllWISE catalogue with machine learning methods
• The phase spiral in Gaia DR3
• What Does the Milky Way Look Like?
• Gaia Data Release 3 Validating the classification of variable Young Stellar Object candidates
• The Radcliffe Wave is Oscillating
• Evidence of a vertical kinematic oscillation beyond the Radcliffe Wave
• A Census of Star Formation in the Outer Galaxy II: The GLIMPSE360 Field
• On the origin of the North Celestial Pole Loop
• Discovery of a coherent, wave-like velocity pattern for the Radcliffe Wave
• Distances to nearby molecular clouds traced by young stars
• Parameters of the Radcliffe wave from masers, radio stars and T Tauri stars
• Kinetic tomography of the Galactic plane within 1.25 kiloparsecs from the Sun. The interstellar flows revealed by HI and CO line emission and 3D dust
• Segments of spiral arms of the Galaxy traced by classical Cepheids: Effects of age heterogeneity
• The parallax and 3D kinematics of water masers in the massive star-forming region G034.43+0.24
• Steady states of the Parker instability
• Radial Wave in the Galactic Disk: New Clues to Discriminate Different Perturbations
• Weather Forecast of the Milky Way: Shear and Stellar feedback determine the lives of Galactic-scale filaments
• Parallax-based Distances to Galactic Hii Regions: Nearby Spiral Structure
• Analysis of Galactic Rotation from Masers based on a Nonlinear Oort Model
• The Solar System's passage through the Radcliffe wave during the middle Miocene
• The Radcliffe Wave as traced by young open clusters: Stellar parameters, activity indicators, and abundances of solar-type members of eight young clusters
• The magnetic field of the Radcliffe Wave: starlight polarization at nearest approach to the Sun
• The Impact of Cosmic Ray Injection on Magnetic Flux Tubes in a Galactic Disk
• Cosmic ray acceleration and non-thermal emission from fast luminous optical transient sources
• Kinematics of T Tauri Stars Close to the Sun from the Gaia DR2 Catalogue
• The Radcliffe wave parameters from data on open star clusters