Hostname: page-component-745bb68f8f-grxwn Total loading time: 0 Render date: 2025-02-03T11:47:08.110Z Has data issue: false hasContentIssue false
  • English
  • Français

Hα Emission Line Profiles in the Spectrum of Algol

Published online by Cambridge University Press:  14 August 2015

C. T. Bolton  and
Donna J. Zubrod
C. T. Bolton
Affiliation:
David Dunlap Observatory, University of Toronto P.O. Box 360, Richmond Hill, Ontario, CANADA L4C 4Y6
Donna J. Zubrod
Affiliation:
David Dunlap Observatory, University of Toronto P.O. Box 360, Richmond Hill, Ontario, CANADA L4C 4Y6

Extract

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.

We have investigated variations in the strength and profile of the Hα emission line in the spectrum of Algol using 145 16 A° mm−1 spectrograms obtained during the period September, 1976 to December, 1977. The Hα emission line profile has been extracted by subtracting the absorption contributions of the three stars in the system. The resulting data set has been analyzed to look for variations related to orbital phase as well as shorter and longer term variations.

Type
V. Algol and Algols
Information
Symposium - International Astronomical Union , Volume 88: Close Binary Stars: Observations and Interpretation , 1980 , pp. 225 - 227
Copyright
Copyright © Reidel 1980