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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Published in | Publications of the Astronomical Society of the Pacific Vol. 89; no. 527; pp. 69 - 70 |
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Main Authors | , |
Format | Journal Article |
Language | English |
Published |
The Astronomical Society of the Pacific
01.02.1977
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Subjects | |
Online Access | Get full text |
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