γ-RAY EMISSION FROM LS I+61 303: THE IMPACT OF BASIC SYSTEM UNCERTAINTIES

被引:28
作者
Sierpowska-Bartosik, Agnieszka [1 ]
Torres, Diego F. [1 ]
机构
[1] CSIC, IEEC, Inst Ciencies Espai, Fac Ciencies, Barcelona 08193, Spain
关键词
gamma rays: observations; gamma rays: theory; X-rays: binaries; MICROQUASAR LS-I+61-303; PARTICLE-ACCELERATION; IRAS OBSERVATIONS; RADIO-EMISSION; PULSAR MODEL; H-ALPHA; BINARY; LS-5039; STARS; WINDS;
D O I
10.1088/0004-637X/693/2/1462
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
LS I +61 303 has been recently detected as a periodic gamma-ray source by the Major Atmospheric Imaging Cerenkov (MAGIC) telescope. A distinctive orbital correlation of the gamma-ray emission was found. This work shows that the range of uncertainties yet at hand in the orbital elements of the binary system LS I +61 303 as well as in the possible assumptions on the stellar wind of the optical companion play a non-negligible role in the computation of opacities to high-energy processes leading to gamma-ray predictions. The geometry influence on the propagation and escape of gamma-ray photons is explored. With this study at hand, we analyze the results of a pulsar wind zone model for the production of gamma-rays and compare it with recent MAGIC observations.
引用
收藏
页码:1462 / 1473
页数:12
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