Last Updated:2025/12/08

When modeling protostar evolution, we found that the radius could not exceed the Hayashi limit for its mass.

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When modeling protostar evolution, we found that the radius could not exceed the Hayashi limit for its mass.

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原始星の進化をモデル化したところ、その質量に対してハヤシ限界(理論上の最大半径)を超えることはできないと分かった。

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