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Updated: Dec 8, 2025

Scattering And Absorption of Light in Planetary Regoliths
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進化した星の風を形作る

L Decin1,2, M Montargès3, A M S Richards4

  • 1Institute of Astronomy, KU Leuven, 3001 Leuven, Belgium. leen.decin@kuleuven.be.

Science (New York, N.Y.)
|September 18, 2020
PubMed
まとめ

バイナリー相互作用は,アシンプトティック・ジャイアント・ブランチ (AGB) の星が惑星性星雲 (PNe) に似た非球形風を発達させる理由を説明するかもしれない. ALMAの観測により これらのAGB風は複雑な形をしていることが分かり この進化を誘導する 二重の伴星が示唆されています

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