Magnetic field amplification in Tycho and other shell-type supernova remnants

H. J. Völk; E. G. Berezhko; L. T. Ksenofontov

doi:10.1051/0004-6361:20042015e

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Volume 444 / No 3 (December IV 2005)

A&A, 444 3 (2005) 893

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Issue		A&A Volume 444, Number 3, December IV 2005


Page(s)		893 - 893
Section		Interstellar and circumstellar matter
DOI		https://doi.org/10.1051/0004-6361:20042015e
Published online		05 December 2005

A&A 444, 893-893 (2005)

Magnetic field amplification in Tycho and other shell-type supernova remnants

H. J. Völk¹, E. G. Berezhko² and L. T. Ksenofontov²

¹ Max-Planck-Institut für Kernphysik, Postfach 103980, 69029 Heidelberg, Germany e-mail: Heinrich.Voelk@mpi-hd.mpg.de
² Yu. G. Shafer Institute of Cosmophysical Research and Aeronomy, 31 Lenin Ave., 678980 Yakutsk, Russia e-mail: [berezhko;ksenofon]@ikfia.ysn.ru

This article has no abstract.

Key words: plasmas / acceleration of particles / ISM: supernova remnants / ISM: cosmic rays / radiation mechanisms: non-thermal / errata, addenda

Erratum to: A&A, 433, 229–240 (2005), DOI: 10.1051/0004-6361:20042015

© ESO, 2005

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