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超新星発生後の密着バイナリ系における12.4日周期
Ping Chen1, Avishay Gal-Yam2, Jesper Sollerman3
1Department of Particle Physics and Astrophysics, Weizmann Institute of Science, Rehovot, Israel. chen.ping@weizmann.ac.il.
Nature
|January 10, 2024
まとめ
天文学者は超新星SN 2022jliを観測し,周期的な光の変化と水素の放出を明らかにした. これは二重星系内の 巨大な恒星が爆発し,その伴星から物質を 蓄積したコンパクトな物体を残したことを示唆しています
科学分野:
- 天文学と天体物理学
- 星の進化について
- 超新星
背景:
- 中性子星や恒星の質量を持つブラックホールは 巨大な星の爆発によって形成されます
- 巨大な恒星はしばしば二重星系に存在するが,二重星系における超新星期のコンパクトな物体の形成の直接的な証拠は稀である.
研究 の 目的:
- 超新星 SN2022jliの性質を調査する
- 超新星残骸の二元性や コンパクトな物体の形成を 探すためだ
主な方法:
- SN 2022jliのフォトメトリックモニタリングにより,光の曲線の変化を検出する.
- Hαを含む,遅い時間の放射のスペクトル分析.
- フェルミ-LATからのガンマ線源データとの相関.
主要な成果:
- SN 2022jliは12.4日間の周期的な波動を示した.
- 遅い時間のスペクトルは,周期的な速度シフトを持つ狭いHα放出を示し,コンパクトな残骸への増殖を示した.
- 新しいフェルミ-LATのガンマ線源は,SN 2022jliの位置とタイミングと一致していることが判明しました.
結論:
- 観測された性質は,SN 2022jliが二重星系にある巨大な恒星から生まれたことを強く示唆しています.
- このコンパクトな残骸は 伴星から質量を蓄積し 超新星の光の曲線を動かし ガンマ線を放出しています
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