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Effects of uniform and differential rotation on stellar pulsations

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dc.creator Deupree, Robert G. (Robert Gaston), 1946-
dc.creator Lovekin, C. C.
dc.creator Clement, M. J.
dc.date.accessioned 2015-04-07T12:57:42Z
dc.date.available 2015-04-07T12:57:42Z
dc.date.issued 2009-03-01
dc.identifier.issn 0004-637X
dc.identifier.uri http://library2.smu.ca/xmlui/handle/01/26026
dc.description Publisher's version/PDF en_CA
dc.description.abstract We have investigated the effects of uniform rotation and a specific model for differential rotation on the pulsation frequencies of 10 M[subscript circled dot] stellar models. Uniform rotation decreases the frequencies for all modes. Differential rotation does not appear to have a significant effect on the frequencies, except for the most extreme differentially rotating models. In all cases, the large and small separations show the effects of rotation at lower velocities than do the individual frequencies. Unfortunately, to a certain extent, differential rotation mimics the effects of more rapid rotation, and only the presence of some specific observed frequencies with well identified modes will be able to uniquely constrain the internal rotation of pulsating stars. en_CA
dc.language.iso en en_CA
dc.publisher American Astronomical Society en_CA
dc.publisher IOP Publishing
dc.relation.uri http://dx.doi.org/10.1088/0004-637X/693/1/677
dc.rights Article is made available in accordance with the publisher’s policy and is subject to copyright law. Please refer to the publisher’s site. Any re-use of this article is to be in accordance with the publisher’s copyright policy. This posting is in no way granting any permission for re-use to the reader/user.
dc.subject.lcsh Stellar oscillations
dc.subject.lcsh Stars -- Rotation
dc.title Effects of uniform and differential rotation on stellar pulsations en_CA
dc.type Text en_CA
dcterms.bibliographicCitation Astrophysical Journal 693(1), 677-690. (2009) en_CA

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