F Ma1, B J Wills

  • 1Prc-Mrc 2nd Floor/R9950, McDonald Observatory and Astronomy Department, University of Texas, Austin, TX 78712, USA. feng@astro.as.utexas.edu

Science (New York, N.Y.)
|June 16, 2001
PubMed
まとめ

ブレーザーは,放射線比の変化を観察することによって検出され,ラジオ騒音クエザーの統一モデルをサポートします. この研究では,クワザーの放射線が10年以上にわたって有意に変化していることが判明しました.

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