@Article{BeckLoHuBeGrWi:1989:StMaFi,
author = "Beck, R. and Loiseau, N. and Hummel, E. and Berkhuijsen, E. M. and
Gr{\"a}ve, R. and Wielebinski, R.",
affiliation = "{Max-Planck-Institut f{\"u}r Radioastronomie} and {Instituto
Nacional de Pesquisas Espaciais (INPE)} and {Max-Planck-Institut
f{\"u}r Radioastronomie / Nuffield Radio Astronomy Laboratories}
and {Max-Planck-Institut f{\"u}r Radioastronomie} and
{Max-Planck-Institut f{\"u}r Radioastronomie /
Max-Planck-Institut f{\"u}r Astronomie} and {Max-Planck-Institut
f{\"u}r Radioastronomie}",
title = "High-resolution polarization observations of M31. 1. Structure of
the magnetic field in the southwestern arm",
journal = "Astronomy \& Astrophysics",
year = "1989",
volume = "222",
pages = "58--68",
keywords = "M31, spiral galaxies, radio continuum, Faraday rotation,
interstellar magnetic fields, polarization.",
abstract = "A region surrounding the main spiral arm southwest of the nucleus
of M31 has been observed with VLA and Effelsberg radio telescopes
and 20.1 and 6.3 cm wavelengths, respectively. The model of a
basic axisymmetric nearly toroidal field in M31 is supported by
the observed rotation measures and intrinsic magnetic field
orientations. The observation of periodic deviations from the
basic axisymmetric field suggest a three-dimensional arc-like
field structure.",
issn = "0004-6361 and 1432-0746",
label = "2987",
language = "en",
targetfile = "1989A+A___222___58B.pdf",
urlaccessdate = "04 maio 2024"
}