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 SlowlyPulsating B Stars. The lack of observed variable HgMn stars suggeststhat some physical process is missing from the models. Somepossibilities are discussed.
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Turcotte, S., Richard, O. Of Variability, or its Absence, in HgMn Stars. Astrophysics and Space Science 284, 225–228 (2003). https://doi.org/10.1023/A:1023243719709
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DOI: https://doi.org/10.1023/A:1023243719709