OB stars TESS phot. & high-resolution spectroscopy
收藏B2FIND2026-04-04 收录
下载链接：
https://b2find.eudat.eu/dataset/8ac9aeb6-8806-5d4b-bdf9-0461408b1169
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Massive stars are predicted to excite internal gravity waves (IGWs) by turbulent core convection and from turbulent pressure fluctuations in their near-surface layers. These...
据预测，大质量恒星可通过其核心的湍流对流，以及近表层的湍流压力涨落激发内部重力波（internal gravity waves, IGWs）。上述……
