The Rotation of the Ap Stars from the Point of View of the Rigid Rotator Model-Reference-Cited by-同舟云学术

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The Rotation of the Ap Stars from the Point of View of the Rigid Rotator Model

Published:1970 Issue: Volume: Page:254-263
ISSN:
Container-title:Stellar Rotation
language:
Short-container-title:

Author:

Preston George W.

Publisher

Springer Netherlands

Link

http://link.springer.com/content/pdf/10.1007/978-94-010-3299-5_28.pdf

Reference39 articles.

1. Babcock, H. W.: 1951, Astrophys. J. 114, 1.

2. Babcock, H. W.: 1956, Astrophys. J. 124, 489.

3. Babcock, H. W.: 1958, Astrophys. J. Suppl. 3, No. 30.

4. Babcock, H. W.: 1960, in Stars and Stellar Systems 6, p. 282.

5. Bahner, K. and Mawridis, L.: 1957, Z. Astrophys. 41, 254.

Cited by 24 articles. 订阅此论文施引文献订阅此论文施引文献，注册后可以免费订阅5篇论文的施引文献，订阅后可以查看论文全部施引文献

1. Long-period Ap stars discovered with TESS data: Cycles 3 and 4;Astronomy & Astrophysics;2024-03

2. Long-period Ap stars discovered with TESS data;Astronomy & Astrophysics;2020-07

3. On the properties of the magnetic Chemically Peculiar B, A, and F-type stars;Proceedings of the International Astronomical Union;2019-06

4. Variation of the magnetic field of the Ap star HD 50169 over its 29-year rotation period;Astronomy & Astrophysics;2019-04

5. Studies of FCAPT uvby Photometry with Period04: The mCP Stars HD 5797, HD 36792, HD 27309, HD 47913, HD 74521, HD 120198, HD 171263, and HD 215441;Publications of the Astronomical Society of the Pacific;2018-03-15

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