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dc.contributor.authorCollier Cameron, A.
dc.contributor.authorBarnes, J.R.
dc.contributor.authorKitchatinov, L.
dc.contributor.authorDonati, J-F.
dc.date.accessioned2008-01-30T10:42:50Z
dc.date.available2008-01-30T10:42:50Z
dc.date.issued2001
dc.identifier.citationCollier Cameron , A , Barnes , J R , Kitchatinov , L & Donati , J-F 2001 , Differential Rotation in Young Low-mass Stars . in In: Procs of 11th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, ASP Conference Series 223 . Astronomical Society of the Pacific , pp. 251-60 .
dc.identifier.isbn1-58381-055-2
dc.identifier.otherPURE: 181378
dc.identifier.otherPURE UUID: cd4113d1-33e1-450b-bd15-fcbd61fa0ccf
dc.identifier.otherdspace: 2299/1477
dc.identifier.urihttp://hdl.handle.net/2299/1477
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/222-252.html--Copyright Astronomical Society of the Pacific
dc.description.abstractMulti-line Doppler imaging methods allow us to image young, rapidly rotating stars brighter than about V = 11.5, with ~ 3 degrees surface resolution. We have recently measured the latitude dependence of the surface rotation rate in three young G and K stars by cross-correlating Doppler images reconstructed from data sets secured several days apart. As a result, new theoretical models of solar and stellar internal rotation can be tested directly against the form, amplitude and spectral-type dependence of differential rotation in both Sun and stars. We present new maps of AB Dor, PZ Tel and RX J1508.6-4423, which all show a solar-like differential rotation pattern and rate of surface shear.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Procs of 11th Cambridge Workshop on Cool Stars, Stellar Systems and the Sun, ASP Conference Series 223
dc.titleDifferential Rotation in Young Low-mass Starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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