水蒸気マザー"Turn-On"は,HII領域のW3 (OH) で使用されています
まとめ
W3(OH) の水蒸気マザー放射は一時的な明るさの上昇を示し,これは単純なマザーモデルによって説明されます. これは,O5星からの短いエネルギー漏れを示唆しています.
科学分野:
- 天体物理学 天体物理学
- ラジオ天文学 ラジオ天文学
背景:
- 水蒸気マザーは,恒星形成領域の重要な探査機である.
- W3(OH) は,よく研究された巨大な恒星形成領域です.
研究 の 目的:
- W3(OH) の水蒸気マザースペクトルの観測された変動性を調査する.
- マザーの強度の変動に起因する物理的プロセスをモデル化するために.
主な方法:
- W3(OH) の水蒸気マザーラインの観測監視.
- 観測された強度の変動を解釈するために,単純なマザーモデルを適用する.
主要な成果:
- マザー光度が8日間で一時的に上昇し,その後4週間にわたって減少する.
- 観測された光の曲線は,突然のエネルギー衝動と一致しています.
結論:
- この変動は,一時的なエネルギー入力を持つマザーモデルで説明できる.
- エネルギー源は,おそらく,塵の中のO5星からの短い"漏れ"である.
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