関連する実験動画
Updated: Jul 18, 2026

06:28
Cerenkov Luminescence Imaging of Interscapular Brown Adipose Tissue
Published on: October 7, 2014
超新星残骸カシオペアAの近くで赤外線が反響している
Oliver Krause1, George H Rieke, Stephan M Birkmann
1Steward Observatory, University of Arizona, 933 North Cherry Avenue, Tucson, AZ 85721, USA. krause@as.arizona.edu
まとめ
スピッツァー宇宙望遠鏡で観測されたカシオペアAの近くの動く構造は,光速に近い速度を示しています. これらの現象は,おそらく超新星残骸の爆発によって加熱された塵からの赤外線エコーである.
科学分野:
- 天文学 天文学
- 天体物理学 天体物理学
- コスミック・フェノメン (宇宙現象)
背景:
- カシオペアAは,よく研究された超新星残骸です.
- 超新星残骸は,恒星の進化と元素の分布を理解するための鍵です.
研究 の 目的:
- カッシオペイア A超新星残骸の周りに観測されたダイナミックな構造を調査するために.
- これらの外部の特徴の性質と速度を決定する.
主な方法:
- スピッツァー宇宙望遠鏡を用いて,カシオペアAの24マイクロメートルの2つの画像を1年間隔で取得した.
- 残骸の殻の外にある構造物の明らかな動きの分析.
- 近赤外線観測を用いた独立した確認.
主要な成果:
- カシオペアAの殻から20弧分に及ぶ移動構造を観測した.
- 個々の特徴は,年間10〜20の弧秒の動きを示した.
- これらの構造は,光の速度に近づく接触速度を示した.
結論:
- 観測された動く構造は,赤外線エコーとして識別されます.
- これらのエコーは,超新星爆発によって加熱された恒星間塵と,カシオペアAの中央のコンパクトオブジェクトからのフレアによって生成されます.
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