Fits to X-ray, radio, and TeV data for the eastern rim of SN 1006

被引：6

作者：

Allen, GE

Houck, JC

Sturner, SJ

机构：

[1] MIT, Space Res Ctr, Cambridge, MA 02139 USA

[2] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA

来源：

HIGH-ENERGY STUDIES OF SUPERNOVA REMNANTS AND NEUTRON STARS | 2004年 / 33卷 / 04期

关键词：

supernova remnants; SN; 1006; X-ray data; synchrotron radiation; inverse compton emission; cosmic rays;

D O I：

10.1016/j.asr.2003.07.027

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

We performed a joint fit to radio, recent Chandra X-ray, and gamma-ray data for the supernova remnant SN 1006 using models of synchrotron and inverse-Compton emission. The results are used to determine the magnetic field strength and the properties of the electron spectrum for the eastern rim of the remnant. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.

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页码：440 / 445

页数：6

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