SpringerLink
Forum Springer Astron. Astrophys.
Forum Whats New Search Orders


Astron. Astrophys. 355, 128-137 (2000)


Table of Contents
Available formats: HTML | PDF | (gzipped) PostScript

Regular magnetic fields in the dwarf irregular galaxy NGC 4449

K.T. Chyy 1, R. Beck 2, S. Kohle 3, U. Klein 3 and M. Urbanik 1

1 Astronomical Observatory, Jagiellonian University, ul Orla 171, 30-244 Kraków, Poland
2 Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, 53121 Bonn, Germany
3 Radioastronomisches Institut der Universität Bonn, Auf dem Hügel 71, 53121 Bonn, Germany

Received 18 November 1999 / Accepted 22 December 1999

Abstract

We present a high-resolution VLA study of the total power and polarized radio continuum emission at 8.46 and 4.86 GHz of the irregular galaxy NGC 4449, known for its weak rotation and non-systematic gas motions. We found strong galaxy-scale regular magnetic fields, which is surprising because of a lack of ordered rotation required for the dynamo action. The strength of the regular field reaches 8 µG and that of the total field 14 µG, comparable to that of the total magnetic field strength in radio-bright spirals. The magnetic vectors in NGC 4449 form radial "fans" in the central region and fragments of a spiral pattern in the galaxy's outskirts. These structures are associated with large regions of systematic Faraday rotation, implying genuine galaxy-scale magnetic fields rather than random ones compressed and stretched by gas flows. The observed pattern of polarization B-vectors is similar to dynamo-type fields in normal spirals. Nonstandard, fast dynamo concepts are required to explain the observed field strengths, though it is unknown what kind of magnetic field geometry can be produced in slowly and chaotically rotating objects. The so far neglected role of magnetic fields for the dynamics and star formation in dwarf irregulars also needs to be revised.

Key words: galaxies: magnetic fields – galaxies: irregular – galaxies: individual: – radio continuum: galaxies – polarization

Send offprint requests to: K. Chyy (chris@oa.uj.edu.pl)

Correspondence to: chris@oa.uj.edu.pl

© European Southern Observatory (ESO) 2000

Online publication: March 17, 2000

helpdesk.link@springer.de