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Pulsations in massive stars: Effect of the atmosphere on the strange mode pulsations

dc.contributor.authorGodart, M.
dc.contributor.authorDupret, M.-A.
dc.contributor.authorNoels, A.
dc.contributor.authorAerts, C.
dc.contributor.authorSimón-Díaz, S.
dc.contributor.authorLefever, K.
dc.contributor.authorPuls, J.
dc.contributor.authorMontalban, J.
dc.contributor.authorVentura, P.
dc.date2010
dc.date.accessioned2016-04-06T08:26:21Z
dc.date.available2016-04-06T08:26:21Z
dc.identifier.urihttps://orfeo.belnet.be/handle/internal/3325
dc.descriptionRecent space observations with CoRoT and ground-based spectroscopy have shown the presence of different types of pulsations in OB stars. These oscillations could be due to acoustic and gravity modes, solar-like oscillations or even other pulsations of large growth rates. We present a first attempt at interpreting the latter as strange modes.
dc.titlePulsations in massive stars: Effect of the atmosphere on the strange mode pulsations
dc.typeConference
dc.subject.frascatiPhysical sciences
dc.audienceScientific
dc.source.titleProceedings of the International Astronomical Union
dc.source.volume6
dc.source.issueS272
dc.source.page503-504
Orfeo.peerreviewedNo
dc.identifier.doi10.1017/S1743921311011185
dc.identifier.scopus2-s2.0-84882791857


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