Year: 2014
Type: article
Abstract: Aims. Two-dimensional magnetohydrodynamic (MHD) simulations are used to model the emission properties of TeV-bright shell-type supernova remnants (SNRs) and to explore their nature.
Source: Astronomy and Astrophysics
Authors: Chuyuan Yang, Siming Liu, Jun Fang, Hui Li
Language: English
Subfield: Nuclear and High Energy Physics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: bronze
OpenAlex ID: W2129221070
