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自转恒星中各向异性的星风物质损失的研究 被引量：1

Anisotropy Losses of Mass due to Steller Wind in the Rotating Stellar
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摘要 通过介绍忽略自转效应的恒星结构的一维模型与一维模型下星风物质损失的成功与不足,给出了考虑自转效应下恒星结构的二维模型与二维模型下星风物质损失。 This paper introduces one dimensional model of the stellar structure without rotational effects and losses of mass due to steller wind in this model,analyses the success and shortcoming of them ,and gives twe demensional model of the stellar structure with rotational effects and losses of mass due to steller wind in this model.
作者 卢媛
机构地区 毕节学院物理系
出处 《毕节学院学报（综合版）》 2009年第8期62-66,共5页 Journal of Bijie University
关键词 自转效应 二维模型 各向异性的星风物质损失 Rotational Effects Two Demensional Model Anisotropy Losses of Mass due to Steller Wind
分类号 O412 [理学—理论物理]
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参考文献10

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同被引文献8

  • 1de Jager C, Nieuwenhuijzen H, Van Der Hucht K A.Mass loss rates in the hertzsprung-russeU diargam [J] .Bull.Inform.C DS., 1988,35:141-142.
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引证文献1

毕节学院学报（综合版）
2009年 第8期

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