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Updated: Apr 25, 2026

Visualization of Low-Level Gamma Radiation Sources Using a Low-Cost, High-Sensitivity, Omnidirectional Compton Camera
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コバルト-56型Ia超新星2014Jからのγ線放射線

E Churazov1, R Sunyaev1, J Isern2

  • 11] Space Research Institute (IKI), Profsouznaya 84/32, Moscow 117997, Russia [2] Max Planck Institute for Astrophysics, Karl-Schwarzschild-Strasse 1, 85741 Garching, Germany.

Nature
|August 29, 2014
PubMed
まとめ

研究者らは,タイプIア超新星2014Jからのガンマ線を検出し,放射性ニッケル-56.6の合成を確認しました. これは,超新星爆発とその噴出物の膨張速度に関する重要なデータを提供します.

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