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- W1491370946 abstract "A number of spectroscopic peculiarities of K giants and other stars which lie in a wedge in the HR diagram are discussed. These peculiarities can be understood in terms of unsteady magnetic flux loops emerging into the stellar atmosphere from beneath the surface." @default.
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- W1491370946 date "1982-01-01" @default.
- W1491370946 modified "2023-09-27" @default.
- W1491370946 title "Discrepant asymmetry stars: The role of unsteady magnetic flux loops in the atmospheres of late-type giant stars" @default.
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