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Acoustic wave driven mass loss in late-type giant stars
1987
Symposium - International astronomical union
Preserved Fulltext
Mass loss generated by radiatively damped acoustic waves is investigated. We find that a persistent wave energy flux leads to extended chromospheres. Mass loss is quite likely produced if the wave field retains a transient character and if large wave periods are used.
doi:10.1017/s0074180900156645
fatcat:rxj45rgvbrhazhpl4osnnp3azy