Published 1998 | Version v1
Journal article

Magnetic Fields and Rotation of Spiral Galaxies

  • 1. Universidad de Granada (Spain)

Description

We present a simplified model in which we suggest that two important galactic problems- the magnetic field configuration at large scales and the flat rotation curve-may be simultaneously explained. A highly convective disc produces a high turbulent magnetic diffusion in the vertical direction, establishing a merging of extragalactic and galactic magnetic fields. The outer disc may then acquire a magnetic energy gradient very close to the gradient required to explain the rotation curve, without the hypotheses of galactic dark matter. Our model predicts symmetries of the galactic field in noticeable agreement with the large scale structure of our Galaxy. (Author) 46 refs

Additional details

Publishing Information

Journal Title
Anales de Fisica (1992)
Journal Volume
94
Journal Issue
2
Journal Page Range
p. 98-102
CODEN
AFISEX

INIS

Country of Publication
Spain
Country of Input or Organization
Spain
INIS RN
30019203
Subject category
S71: CLASSICAL AND QUANTUM MECHANICS, GENERAL PHYSICS;
Descriptors DEI
GALAXIES; MAGNETIC FIELDS; ROTATION; SPIRAL CONFIGURATION
Descriptors DEC
CONFIGURATION