CA ii EMISSION VARIABILITY IN BY DRACONIS

Photoelectric spectrophotometry of the Can K emission line in the flare star BY Dra during 1975 shows no evidence for variability over the 3ḍ8 rotation period. Apparently the K-line emission is produced uniformly over the stellar surface, and is not localized in plage regions. Concurrent variations...

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Bibliographic Details
Published inPublications of the Astronomical Society of the Pacific Vol. 89; no. 527; pp. 69 - 70
Main Authors BOPP, BERNARD W., FERLAND, GARY
Format Journal Article
LanguageEnglish
Published The Astronomical Society of the Pacific 01.02.1977
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