まとめ
前面の銀河の恒星による重力レンズ化は,BL Lacertaeオブジェクトを説明する可能性があります. この現象は,背景の光学的に暴力的な変数クエーザーを増幅し,観測されたBL Lac赤偏移分布に影響を与えます.
科学分野:
- 天文学 天文学
- 天体物理学 天体物理学
- コスモロジー・コスモロジーとは
背景:
- BL Lacertaeオブジェクト (BL Lacs) は,無線クエーサーである.
- 以前の仮説では,BL Lacsは重力レンズ化された光学的に暴力的な変数 (OVV) 準星であると考えられていた.
- この仮説は,BL LacsとOVVクエーザーの一般的な類似性に基づいていた.
研究 の 目的:
- BL Lacsが重力レンズ付きOVVクエーサーであるという仮説を検証する.
- BL Lac赤偏移の観測された分布を説明するために.
- マイクロレンズとして作用する銀河の特徴を特定する.
主な方法:
- 最近観測されたBL Lacオブジェクトの分析.
- BL湖の空間的宇宙分布の調査.
- 前面の銀河の恒星による重力レンズ効果のモデル化.
主要な成果:
- 証拠によると,いくつかのBL湖はレンズ化されたOVVクエーサーであり,前景の円銀河が観測されている.
- 観測されたBL Lac赤偏移分布は,重力レンズなしで説明するのは困難です.
- マイクロレンズ銀河は,0.05-0.10と遠くのクワサール近くにある2つの赤道移転ピークで出現すると予測されています.
結論:
- 前面の銀河の恒星による重力レンズは,BL Lacオブジェクトの重要な部分の妥当な説明です.
- このレンズメカニズムは,観測されたBL Lac赤偏移分布を宇宙学的モデルと調和させるのに役立ちます.
- この研究は,マイクロレンズとして作用する銀河の特定の赤道移転範囲を予測しています.
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