Titlebook: Stellar Rotation; Proceedings of the I Arne Slettebak Conference proceedings 1970 D. Reidel Publishing Company, Dordrecht, Holland 1970 sta

Extraneous

书目名称Stellar Rotation影响因子(影响力)




书目名称Stellar Rotation影响因子(影响力)学科排名




书目名称Stellar Rotation网络公开度




书目名称Stellar Rotation网络公开度学科排名




书目名称Stellar Rotation被引频次




书目名称Stellar Rotation被引频次学科排名




书目名称Stellar Rotation年度引用




书目名称Stellar Rotation年度引用学科排名




书目名称Stellar Rotation读者反馈




书目名称Stellar Rotation读者反馈学科排名

CHAFE

On the Effect of Rotation on Stellar Absorption Lineseric parameters of a rapidly rotating star seen pole-on are very similar to those of a non-rotating star of the same mass, this may cause significant errors in abundance determinations, especially for Eu-type elements. The aspect effect on the central intensity of two EuII lines of different strengths is also studied.

严重伤害

Rotation and Macroturbulence in Supergiant Starsportant a broadening agent as large-scale mass motion. In the middle B and A stars turbulence dominates but there still is an appreciable contribution from rotation. (2) In spite of the fact that the stars observed seem to be losing mass, there is no strong evidence for significant angular momentum loss.

GULF

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充气女

PARA

Rotational Velocities of Evolved A and F Starstent with the hypothesis of stellar rotation in completely uncoupled shells for stars that have expanded in radius by less than a factor of four. They do, however, support the hypothesis of solid-body rotation for these stars. The data for the giant stars are discussed, but no firm conclusions about

amorphous

GROG

Evolution of Rapidly Rotating B-Type Stars and Roxburgh and Strittmatter (1965) how seriously the spectrum of a star may be affected by rotation. However, before atmospheric models for rotating stars can be computed, the results of corresponding interior models have to be available. For polytropic configurations a great many rotating interi

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