SYNCHROTRON EMISSION FROM TYPE-I SUPERNOVA-REMNANTS

被引：0
作者：
AMMOSOV, AE
KSENOFONTOV, LT
NIKOLAEV, VS
PETUKHOV, SI
机构：
来源：
ASTRONOMY LETTERS-A JOURNAL OF ASTRONOMY AND SPACE ASTROPHYSICS | 1994年 / 20卷 / 02期
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D O I：
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中图分类号：
P1 [天文学];
学科分类号：
0704 ;
摘要：
A model of synchrotron emission of the electrons accelerated by the outer shock wave in the magnetic field of a supernova remnant is calculated; the magnetic field is the modified interstellar field. This model can describe the synchrotron emission from type I supernova remnants. A comparison with observations shows that the results of calculations are in satisfactory agreement with data on the remnants of SN 1006 and Tycho's SN in the frequency range nu = 10(9) - 10(18) Hz.
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页码：157 / 162
页数：6
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