Convection: A Seismological Perspective

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dc.contributor.utaustinauthorMontgomery, M.H.en
dc.creatorMontgomery, M. H.en
dc.date.accessioned2015-04-16T14:47:53Zen
dc.date.available2015-04-16T14:47:53Zen
dc.date.issued2007-11en
dc.description.abstractI present an overview of the close relationship which convection and stellar pulsation share. This includes the driving, damping, and modulation of oscillations in stars such as the Sun, other solar-type stars, the >classical> pulsators (e.g., Cepheids, RR Lyrae), as well as more recent results from the realm of pulsating white dwarf stars.en
dc.description.departmentAstronomyen
dc.identifier.citationM. H. Montgomery. AIP Conference Proceedings 948, 99 (Nov., 2007); doi: 10.1063/1.2819017en
dc.identifier.doi10.1063/1.2819017en
dc.identifier.issn0094-243Xen
dc.identifier.issn978-0-7354-0462-5en
dc.identifier.urihttp://hdl.handle.net/2152/29436en
dc.language.isoEnglishen
dc.relation.ispartofserialUnsolved Problems in Stellar Physics: A Conference in Honour of Douglas Goughen_US
dc.rightsAdministrative deposit of works to UT Digital Repository: This works author(s) is or was a University faculty member, student or staff member; this article is already available through open access or the publisher allows a PDF version of the article to be freely posted online. The library makes the deposit as a matter of fair use (for scholarly, educational, and research purposes), and to preserve the work and further secure public access to the works of the University.en
dc.subjectconvectionen
dc.subjectsun : oscillationsen
dc.subjectsun : generalen
dc.subjectwhite dwarfsen
dc.subjectsolar pulsational stabilityen
dc.subjectzz-ceti starsen
dc.subjectfrequenciesen
dc.subjectmodesen
dc.subjectdepthen
dc.subjectzoneen
dc.subjectastronomy & astrophysicsen
dc.titleConvection: A Seismological Perspectiveen
dc.typeArticleen

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