BIMA observations of linear polarization in Sagittarius A* at 112 GHz

被引:26
作者
Bower, GC
Wright, MCH
Falcke, H
Backer, DC
机构
[1] Natl Radio Astron Observ, Socorro, NM 87801 USA
[2] Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA
[3] Univ Calif Berkeley, Radio Astron Lab, Berkeley, CA 94720 USA
[4] Max Planck Inst Radioastron, D-53121 Bonn, Germany
基金
美国国家科学基金会;
关键词
galaxies : active; Galaxy : center; polarization; radiation mechanisms : nonthermal; scattering;
D O I
10.1086/323180
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report here Berkeley-Illinois-Maryland Association array observations of linear polarization in Sagittarius A*, the compact radio source in the Galactic center. These observations had a resolution of 20" x 5" oriented north-south. We do not detect linear or circular polarization at a level of 1.8% (1 sigma) at 112 GHz. This puts a new constraint on models that show a sharp change in linear polarization fraction at 100 GHz.
引用
收藏
页码:L103 / L106
页数:4
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