Hostname: page-component-7479d7b7d-wxhwt Total loading time: 0 Render date: 2024-07-11T14:10:15.457Z Has data issue: false hasContentIssue false
  • English
  • Français

Some Hypothesized Observational Aspects of Magnetic Fields in Protoplanetary Nebulae

Published online by Cambridge University Press:  19 July 2016

G. Pascoli
G. Pascoli*
Affiliation:
Faculté des Sciences, Department of Physique, Amiens, France

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

Polarization mapping of some reflection nebulae (e.g., NGC 6729) reveals parallel bands of polarization vectors across pre-main sequence stars (Ward-Thomson et al. 1985, Mon. Not. R. Astr. Soc., 215). These authors have suggested a model in which the bands would be. Explained by dust discs, the grains being aligned by toroidal magnetic fields ∼ 102 μG.

Type
V. Origin of Planetaries
Information
Symposium - International Astronomical Union , Volume 131: Planetary Nebulae , 1989 , pp. 455
Copyright
Copyright © Kluwer 1989