Of Variability, or its Absence, in HgMn Stars

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dc.creatorTurcotte, S.
dc.creatorRichard, O.
dc.date2002-10-18
dc.date.accessioned2026-07-07T02:05:46Z
dc.date.available2026-07-07T02:05:46Z
dc.descriptionCurrent 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.
dc.descriptionTo be published in Asteroseismology in the HR Diagram, proceedings of a conference held in Porto, 1-5 July 2002. $ pages, 3 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0210442
dc.identifierhttp://arxiv.org/abs/astro-ph/0210442
dc.identifierAstrophys.Space Sci. 284 (2003) 225-228
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/5202
dc.subjectAstrophysics
dc.titleOf Variability, or its Absence, in HgMn Stars
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