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

Home

All issues

Volume 444 / No 3 (December IV 2005)

A&A, 444 3 (2005) 893

Abstract

Free Access

Erratum

This article is an erratum for:
[https://doi.org/10.1051/0004-6361:20042015]

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

© ESO, 2005

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.

First page of the article