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Constraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observations
dc.contributor.authorHaskell, Brynmoren_US
dc.contributor.authorDegenaar, Nathalieen_US
dc.contributor.authorHo, Wynn C. G.en_US
dc.date.accessioned2012-07-12T17:25:45Z
dc.date.available2013-09-03T15:38:27Zen_US
dc.date.issued2012-07-21en_US
dc.identifier.citationHaskell, Brynmor; Degenaar, Nathalie; Ho, Wynn C. G. (2012). "Constraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observations." Monthly Notices of the Royal Astronomical Society 424(1). <http://hdl.handle.net/2027.42/92112>en_US
dc.identifier.issn0035-8711en_US
dc.identifier.issn1365-2966en_US
dc.identifier.urihttps://hdl.handle.net/2027.42/92112
dc.description.abstractRapidly rotating neutron stars in low‐mass X‐ray binaries may be an interesting source of gravitational waves (GWs). In particular, several modes of stellar oscillation may be driven unstable by GW emission, and this can lead to a detectable signal. Here we illustrate how current X‐ray and ultraviolet observations can constrain the physics of the r‐mode instability. We show that the core temperatures inferred from the data would place many systems well inside the unstable region predicted by standard physical models. However, this is at odds with theoretical expectations. We discuss different mechanisms that could be at work in the stellar interior, and we show how they can modify the instability window and make it consistent with the inferred temperatures.en_US
dc.publisherWiley Periodicals, Inc.en_US
dc.publisherBlackwell Publishing Ltden_US
dc.subject.otherGravitational Wavesen_US
dc.subject.otherX‐Rays: Binariesen_US
dc.subject.otherStars: Neutronen_US
dc.titleConstraining the physics of the r‐mode instability in neutron stars with X‐ray and ultraviolet observationsen_US
dc.typeArticleen_US
dc.rights.robotsIndexNoFollowen_US
dc.subject.hlbsecondlevelAstronomyen_US
dc.subject.hlbtoplevelScienceen_US
dc.description.peerreviewedPeer Revieweden_US
dc.contributor.affiliationumDepartment of Astronomy, University of Michigan, 500 Church Street, Ann Arbor, MI 48109, USAen_US
dc.contributor.affiliationotherSchool of Mathematics, University of Southampton, Southampton SO17 1BJen_US
dc.contributor.affiliationotherAstronomical Institute ‘Anton Pannekoek’, University of Amsterdam, Science Park 904, 1098 XH Amsterdam, the Netherlandsen_US
dc.description.bitstreamurlhttp://deepblue.lib.umich.edu/bitstream/2027.42/92112/1/j.1365-2966.2012.21171.x.pdf
dc.identifier.doi10.1111/j.1365-2966.2012.21171.xen_US
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