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Henri M J Boffin1, Brent Miszalski, Thomas Rauch

  • 1European Southern Observatory (ESO), Casilla 19001, Santiago, Chile. hboffin@eso.org

Science (New York, N.Y.)
|November 10, 2012
PubMed
まとめ

バイナリー星の相互作用,特にプレセッシング・アクレション・ディスクは,惑星性星雲の非球形の形状を説明する可能性が高い. この研究は,フレミング1システムにおけるこのシナリオを確認し,それを示唆しています.

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