Hostname: page-component-5c6d5d7d68-pkt8n Total loading time: 0 Render date: 2024-08-17T01:10:32.636Z Has data issue: false hasContentIssue false
  • English
  • Français

18. Stellar magnetic fields

Published online by Cambridge University Press:  18 July 2016

Horace W. Babcock
Horace W. Babcock*
Affiliation:
Mount Wilson and Palomar Observatories, Pasadena, California, U.S.A.

Abstract

Core share and HTML view are not available for this content. However, as you have access to this content, a full PDF is available via the ‘Save PDF’ action button.

A report is given of a ten-year observational program directed toward the discovery and investigation of the magnetic fields of stars through the Zeeman effect in their spectra. The emphasis has been on the sharp-line stars of type A, of which ten have been found to show irregular magnetic fluctuations without reversal of polarity, ten others to fluctuate irregularly with occasional reversals of polarity, and six to show essentially periodic variations; of the latter group, four are large-amplitude reversers with periods near one week.

Type
Part III: Stellar Magnetism
Information
Symposium - International Astronomical Union , Volume 6: Electromagnetic Phenomena in Cosmical Physics , 1958 , pp. 161 - 165
Copyright
Copyright © Cambridge University Press 1958 

References

1. Elsasser, W. M. Rev. Mod. Phys. 28, 135, 1956.Google Scholar
2. Morgan, W. W. Publ. Yerkes Obs. 7, pt. 3, 1935.Google Scholar
3. Deutsch, A. J. Astrophys. J. 105, 283, 1947.Google Scholar
4. Deutsch, A. J. Publ. Astr. Soc. Pacif. 68, 92, 1956.Google Scholar
5. Babcock, H. W. and Cowling, T. G. Mon. Not. R. Astr. Soc. 113, 357, 1953.Google Scholar
6. Babcock, H. W. ‘A Catalog of Magnetic Stars’, Astrophys. J. , Suppl. no. 30, 1958.Google Scholar