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N体計算から、球状星団中の潮汐破壊を研究。潮汐破壊はコア重力崩壊球状星団中で多く発生し、潮汐破壊された恒星の25%はblue straggler星になる。また流体計算から潮汐崩壊をモデル化し、中性子星ならミリ秒パルサーになる可能性も示唆された
https://arxiv.org/abs/2204.07169
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論文概要
N体計算から、球状星団中の潮汐破壊を研究。潮汐破壊はコア重力崩壊球状星団中で多く発生し、潮汐破壊された恒星の25%はblue straggler星になる。また流体計算から潮汐崩壊をモデル化し、中性子星ならミリ秒パルサーになる可能性も示唆された
論文を理解する上で重要な図など
論文リンク
https://arxiv.org/abs/2204.07169
The text was updated successfully, but these errors were encountered: