ジェネシスにおけるラジオミリ秒パルサーのスピンダウン
1Argelander-Institut für Astronomie, Universität Bonn, Bonn, Germany. tauris@astro.uni-bonn.de
まとめ
中性子星からのブレーキトルク
科学分野:
- * 天体物理学
- * 恒星の進化について
- * 中性子星物理学
背景:
- *ミリ秒パルサーは,バイナリー伴星からの質量蓄積によって spun upされた古い中性子星です.
- *初期のスピン進化を理解するには,質量移転終了時に膨張する磁気圏を分析する必要があります.
研究 の 目的:
- * 膨張する磁気圏が中性子星のスピン進化に与える影響を調査する.
- * 観測されたスピン分布の違いと,ミリ秒パルサーの年齢差異を説明するために.
主な方法:
- * バイナリ恒星進化の計算を行った.
- * 伴星ロシェの葉分離後の中性子星のブレーキングトルクを分析した.
主要な成果:
- *ブレーキトルクは,パルサーの回転エネルギーの50%以上を消耗させることができる.
- *このエネルギー消耗は,X線パルサーとラジオパルサーのスピン分布の違いを説明する可能性がある.
結論:
- *ブレーキ・トルク・メカニズムは,ミリ秒パルサー・スピンの進化を理解するために極めて重要です.
- *このメカニズムは,パルサーのスピン分布と年齢推定の不一致を解決する可能性がある.
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