Hostname: page-component-7bb8b95d7b-cx56b Total loading time: 0 Render date: 2024-09-29T17:53:05.146Z Has data issue: false hasContentIssue false
  • English
  • Français

Rapid Spectral Variations in Be Stars — New Techniques and Results

Published online by Cambridge University Press:  12 April 2016

J. B. Hutchings ,
G. A. H. Walker  and
J. R. Auman
J. B. Hutchings
Affiliation:
Dominion Astrophysical Observatory
G. A. H. Walker
Affiliation:
University of British Columbia
J. R. Auman
Affiliation:
University of British Columbia

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.

High resolution spectral scans of some Be stars, taken with an Isocon television camera, show changes in the Ha line profile in times of the order of a minute or less.

Type
IV. Duplicity and its Consequences among the Intrinsic Variable Stars
Information
International Astronomical Union Colloquium , Volume 15: New Directions and Frontiers in Variable Stars Research , 1971 , pp. 279 - 285
Copyright
Copyright © Cambridge University Press 1971

References

Bahng, J. D. R., 1971, Ap. J. 187, L75.Google Scholar
Bohlin, R. C., 1970, Ap. T., 162, 571.Google Scholar
Hutchings, J. B., 1970, Mon. Not. R.A.S. 150, 55.CrossRefGoogle Scholar
Hutchings, J. B., 1971, Mon. Not. R.A.S. 152, 109.Google Scholar
Walker, G. A. H., Auman, J. R., Buchholz, V., Goldberg, B., and Isherwood, B., 1971, Publ. Roy. Obs. Edinburgh, 8, 86.Google Scholar