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惑星形成円盤における重力不安定性

Jessica Speedie1, Ruobing Dong2,3, Cassandra Hall4,5

  • 1Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada. jspeedie@uvic.ca.

Nature
|September 4, 2024
PubMed
まとめ

重力不安定は 崩壊した円盤の断片から直接惑星を形成する可能性があります ABオーリゲー円盤の動力学的な証拠は,この惑星形成理論を支持し,その恒星に相対して巨大な円盤があることを示唆している.

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