Evolution of the magnetic fields of main-sequence CP-stars. II-Reference-Cited by-同舟云学术

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Evolution of the magnetic fields of main-sequence CP-stars. II

Published:2013-09 Issue:3 Volume:56 Page:407-420
ISSN:0571-7256
Container-title:Astrophysics
language:en
Short-container-title:Astrophysics

Author:

Glagolevskij Yu. V.

Publisher

Springer Science and Business Media LLC

Subject

Astronomy and Astrophysics

Link

http://link.springer.com/content/pdf/10.1007/s10511-013-9295-4.pdf

Reference41 articles.

1. Yu. V. Glagolevskij, Astrofizika 56, 189 (2013).

2. Yu. V. Glagolevskij, Astrofizika 55, 369 (2012).

3. E. Parker, Cosmic Magnetic Fields, vol. 1 [Russian translation], Mir, Moscow (1982), p. 33.

4. Yu. V. Glagolevskij and E. Gerth, Magnetic stars, Nizhny Arkhyz (2011), p. 153.

5. Yu. V. Glagolevskij and G. A. Chuntonov, Byull. SAO 51, 88 (2001).

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1. Secular Stability of the Magnetic Structures of Magnetic Stars. II;Astrophysics;2020-09

2. Evolutionary Features and Other Characteristics of Magnetic Stars with Helium Anomalies (He-r, He-w);Astrophysical Bulletin;2020-04

3. Progress in Studies of the Evolution of the Magnetic Fields of CP-Stars. II.;Astrophysics;2018-11-03

4. Probable Inner Magnetic Structures of Magnetic Stars. I;Astrophysical Bulletin;2018-04

5. General properties of magnetic CP stars;Astrophysical Bulletin;2017-07

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