新生型のIa型超新星からの強い紫外線パルスです
Yi Cao1, S R Kulkarni2, D Andrew Howell3
1Astronomy Department, California Institute of Technology, Pasadena, California 91125, USA.
Nature
|May 22, 2015
まとめ
観測は,タイプIア超新星からの強い紫外線放射を明らかにし,単一の変性原始チャンネルの証拠を提供します. この発見は,これらの宇宙爆発の起源と,宇宙の距離を測定する際の用途を説明するのに役立ちます.
科学分野:
- 天文学と天体物理学について
- コスモロジー・コスモロジーとは
背景:
- タイプIア超新星は,宇宙学的距離を測定するために不可欠です.
- 彼らの祖先の正確な性質,特に白矮星系は,依然として活発な研究分野です.
- シングル・デジェネレート・チャネル・モデルは,白矮星が伴星から物質を蓄積していることを示唆している.
研究 の 目的:
- Ia型超新星の前身系を調査する.
- シングル・デジェネレート・チャネル・モデルを支持または反証する観察的証拠を集めること.
主な方法:
- スウィフト宇宙望遠鏡を使って観測.
- 爆発から4日以内にタイプIア超新星からの紫外線放射データを分析した.
主要な成果:
- 超新星発生の直後,強烈で減少する紫外線放射の検出.
- 観測された放射パターンは,射出物-伴星相互作用の理論的予測と一致しています.
結論:
- この発見は,単一の変性チャンネルが,いくつかのタイプIア超新星の前身経路としての説得力のある観測証拠を提供します.
- これは,宇宙学の標準的なキャンドルとしてタイプIア超新星の使用を支持します.
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