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Published December 1967 | Published
Journal Article Open

Equivalent Width of Hα in Late-Type Stars

Abstract

The use of the equivalent width of Ha as a luminosity criterion for late-type stars is investigated. The method is found to be no more accurate than MK luminosity classifications. Two spectrograms are presented which indicate a change in the Ha equivalent width in 22 Vul over a three-year period.

Additional Information

© 1967. The Astronomical Society of the Pacific. Received August 8, 1967. I am indebted to Dr. R. P. Kraft for the use of the spectrograms taken by him in 1963.

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Published - Weistrop_1967_PASP_79_546.pdf

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Created:
August 19, 2023
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October 18, 2023