中性子星 の 熱核 爆発 は,その 噴射 の 速さ を 明らか に する
Thomas D Russell1, Nathalie Degenaar2, Jakob van den Eijnden3,4
1Institute of Space Astrophysics and Cosmic Physics, INAF, Palermo, Italy. thomas.russell@inaf.it.
Nature
|March 28, 2024
まとめ
科学者は初めて ニュートロン星からのジェットの速度を測定しました これらのコンパクトジェットは ブラックホールのジェットよりも遅いので ジェットが発射される方法について 新たな洞察を与えてくれます
科学分野:
- 天体物理学
- 高エネルギー天体物理学
背景:
- 相対論的ジェットは 蓄積や大災害における 重要な現象です
- これらのジェット機の発射メカニズムは 未知のままです
- ニュートロン星のジェット速度を測定することで, 蓄積の流れや 恒星に固定された磁場を区別することができます.
研究 の 目的:
- ニュートロン星から発する 圧縮ジェットの速度を測るため
- ジェット特性に対する蓄積率の影響を調査する.
- 主要なジェット発射機構を理解するために
主な方法:
- I型X線爆発の後のジェット放射の明るいフレアを観察する.
- ジェットフレアと 増加した質量増加率の相関関係
- 観測したフレアを使って ジェット速度を測定する
主要な成果:
- I型X線爆発のすぐ後のジェット放射で 明確なフレアが観測された.
- 中性子星のコンパクトジェット速度を測定しました.
- これらのジェットは ブラックホールのジェットよりも 比較的遅いことが分かりました
結論:
- タイプIのX線爆発は一時的に 蓄積率を高め 観測可能なジェットフレアを誘発します
- 測定されたジェット速度は,ジェット打ち上げメカニズムを研究するための新しい方法を提供します.
- 中性子星のジェット速度は ブラックホールのジェットよりも遅いので 異なるパワーメカニズムを示唆しています
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