マグネタールSGR 1900+14の周りの赤外線リング
S Wachter1, E Ramirez-Ruiz, V V Dwarkadas
1Spitzer Science Center, California Institute of Technology, Pasadena, California 91125, USA. wachter@ipac.caltech.edu
Nature
|May 30, 2008
まとめ
天文学者は,磁星SGR 1900+14の周りに赤外線環を発見しました. このリングは,磁星が巨大な恒星から発生し,巨大なフレアによって形成されるという理論を支持しています.
科学分野:
- 天文学と天体物理学について
- 高エネルギー天体物理学 高エネルギー天体物理学
- 中性子星物理学 中性子星物理学
背景:
- マグネタは,電波パルサーとは異なり,非常に強い磁場を持つ中性子星です.
- 以前の研究では,磁星と巨大な祖先星との関連が示唆されていた.
- マグネタールと他の中性子星の間の進化的関係は不明である.
研究 の 目的:
- マグネタールSGR 1900+14.を囲む赤外線環の性質を調査する.
- 観測された環構造の起源と形成機構を決定する.
- マグネタールと巨大な恒星とのつながりを固めるため.
主な方法:
- マグネタールSGR 1900+14の赤外線画像を用いた観測.
- リングの形状,サイズ,エネルギー分析.
- 観測データと恒星の進化と磁気フレアの理論モデルを比較する.
主要な成果:
- マグネタール周りの円形赤外線環または殻の発見 SGR 1900+14.
- リングの特徴は,標準的な恒星の質量損失や超新星残骸の進化と矛盾しています.
- 1998年に発生した巨大な磁星フレアによって作られた塵のない空洞の理論モデルが,リングの寸法を正確に予測しています.
結論:
- 観測された赤外線リングは,磁星SGR 1900+14からの巨大なフレアの結果である可能性が高い.
- この発見は,SGR 1900+14が巨大な恒星群と関連していることを示す強力な証拠を提供します.
- この研究は,磁星と巨大な恒星の祖先の間のリンクを固める.
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