Abstract
Current models and observations of variability in HgMn stars disagree. We present here the models that argue for pulsating HgMn stars with properties similar to those of Slowly Pulsating B Stars. The lack of observed variable HgMn stars suggests that some physical process is missing from the models. Some possibilities are discussed.
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© 2003 Springer Science+Business Media Dordrecht
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Turcotte, S., Richard, O. (2003). Of Variability, or Its Absence, in HgMn Stars. In: Thompson, M.J., Cunha, M.S., Monteiro, M.J.P.F.G. (eds) Asteroseismology Across the HR Diagram. Springer, Dordrecht. https://doi.org/10.1007/978-94-017-0799-2_29
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DOI: https://doi.org/10.1007/978-94-017-0799-2_29
Publisher Name: Springer, Dordrecht
Print ISBN: 978-90-481-6241-3
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