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Updated: May 11, 2026

Theoretical Calculation and Experimental Verification for Dislocation Reduction in Germanium Epitaxial Layers with Semicylindrical Voids on Silicon
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コンパクトなバイナリ星であるSS Cygniまでの正確な幾何学的な距離は,蓄積円盤理論を正当化している

J C A Miller-Jones1, G R Sivakoff, C Knigge

  • 1International Centre for Radio Astronomy Research, Curtin University, Perth, WA 6845, Australia. james.miller-jones@curtin.edu.au

Science (New York, N.Y.)
|May 25, 2013
PubMed
まとめ

精密な距離測定により,SS Cygniはこれまで考えられていたよりも近くにあることが明らかになりました. この発見は,矮星新星に対する蓄積円盤理論に対する大きな課題を解決する.

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