V

R Sahai1, M Morris, G R Knapp

  • 1Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, California 91109, USA. raghvendra.sahai@jpl.nasa.gov

Nature
|November 25, 2003
PubMed
まとめ

天文学者は,アシンプトティックな巨大分岐星V Hydraeから新しいジェットを発見し,非球状惑星星雲の形成に不可欠な高速流出の直接的な証拠を提供しました. この発見は,仲間星の周りの蓄積円盤を含むモデルを裏付けている.

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