2D axisymmetric model of particle acceleration in colliding shock flows system

17th Russian Youth Conference on Physics and Astronomy

物理学;天文学

Gladilin, P.E.^1 ; Bykov, A.M.^1 ; Osipov, S.M.^1 ; Romanskiy, V.I.^1

Ioffe Physical-Technical Institute of the Russian Academy of Sciences, Saint-Petersburg, Russia^1

关键词: 2d axisymmetric models;    Analytical calculation;    Emission spectrums;    Particle acceleration;    Plane-parallel model;    Star clusters;    Supernova remnants;    Three-dimensional structure;   

Others  :  https://iopscience.iop.org/article/10.1088/1742-6596/661/1/012004/pdf
DOI  :  10.1088/1742-6596/661/1/012004

学科分类：天文学(综合)

来源: IOP

【 摘 要 】

We present the 2D axisymmetric model of particle acceleration at colliding shocks from supernova remnant and stellar wind from the nearby star. The model is the expansion of the previously developed plane-parallel model and takes into account three three-dimensional structure of the stellar wind and the supernova remnant shock. Numerical and analytical calculations provides the energetic and spatial distributions of the particles accelerated by colliding shock flows system. The presented model can be used in calculations of the emission spectra of different stellar associations and star clusters with colliding shock flows.