Of Variability, or its Absence, in HgMn Stars

Astronomy and Astrophysics – Astrophysics

Scientific paper

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To be published in Asteroseismology in the HR Diagram, proceedings of a conference held in Porto, 1-5 July 2002. $ pages, 3 fi

Scientific paper

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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