MULTIMESSENGER MODEL FOR THE STARBURST GALAXY M82

被引：59
|
作者：
de Cea del Pozo, Elsa [1 ]
Torres, Diego F. [1 ]
Rodriguez Marrero, Ana Y. [1 ]
机构：
[1] CSIC, IEEC, Inst Ciencies Espai, Fac Ciencies, Barcelona 08193, Spain
来源：
ASTROPHYSICAL JOURNAL | 2009年 / 698卷 / 02期
关键词：
galaxies: individual (M82); galaxies: starburst; gamma rays: observations; gamma rays: theory; neutrinos; GAMMA-RAY EMISSION; HIGH-ENERGY EMISSION; HUBBLE-SPACE-TELESCOPE; COSMIC-RAY; STAR-FORMATION; SUPERNOVA-REMNANTS; MAGNETIC-FIELDS; HIGH-RESOLUTION; CONTINUUM OBSERVATIONS; SECONDARY ELECTRONS;
D O I：
10.1088/0004-637X/698/2/1054
中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
In this paper, a consistent model of the multifrequency emission of the starburst galaxy M82, from radio to gamma-rays, is presented and discussed. Predictions for observations with Fermi, MAGIC II/VERITAS, and Cherenkov Telescope Array telescopes are made. The model is also used to self-consistently compute the (all flavors) emission of neutrinos resulting from this starburst galaxy. This can be used in considerations of diffuse contributions of such objects.
引用
收藏
页码：1054 / 1060
页数：7
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