LEADER 03545nam 2200601Ia 450 001 9910143966803321 005 20200520144314.0 010 $a9783540878315 010 $a3540878319 024 7 $a10.1007/978-3-540-87831-5 035 $a(CKB)1000000000546959 035 $a(SSID)ssj0000319876 035 $a(PQKBManifestationID)11247508 035 $a(PQKBTitleCode)TC0000319876 035 $a(PQKBWorkID)10338840 035 $a(PQKB)10002663 035 $a(DE-He213)978-3-540-87831-5 035 $a(MiAaPQ)EBC3063754 035 $a(PPN)132868431 035 $a(EXLCZ)991000000000546959 100 $a20081126d2009 uy 0 101 0 $aeng 135 $aurnn|008mamaa 181 $ctxt 182 $cc 183 $acr 200 04$aThe rotation of sun and stars /$fJ.-P. Rozelot, C. Neiner (Eds.) 205 $a1st ed. 2009. 210 $aBerlin ;$aHeidelberg $cSpringer-Verlag$d2009 215 $a1 online resource (X, 264 p. 118 illus., 28 illus. in color.) 225 1 $aLecture notes in physics,$x0075-8450 ;$v765 300 $aBibliographic Level Mode of Issuance: Monograph 311 08$a9783642099649 311 08$a3642099645 311 08$a9783540878308 311 08$a3540878300 320 $aIncludes bibliographical references and index. 327 $aThe Sun: A Slowly Rotating Star -- What Is Coming: Issues Raised from Observation of the Shape of the Sun -- Effects of Rotation on Stellar p-Mode Frequencies -- Approaching the Low-Frequency Spectrum of Rotating Stars -- The Rotation of the Solar Core -- Physics of Rotation in Stellar Models -- Long Baseline Interferometry of Rotating Stars Across the HR Diagram: Flattening, Gravity Darkening, Differential Rotation -- Is the Critical Rotation of Be Stars Really Critical for the Be Phenomenon? -- On the Rotation of A-Type Stars -- The Solar Magnetic Field: Surface and Upper Layers, Network and Internetwork Field. 330 $aThe Sun and stars rotate in different ways and at different rates of velocity, and knowledge of how they rotate is important in understanding the formation and evolution of stars and their structure. The wide variety of stars offers an equally wide variety of rotation rates and rotational evolution. From the slowly rotating stars to stars rotating close to their breakup velocities, different techniques and models have to be developed to study rotation and its effects on physical aspects of stars. In fact, one currently witnesses a complete renewal of astrophysical ideas about stellar rotation, mainly due to the development of new models including high-order effects of rotation and magnetism. This book, while not attempting to answer all questions about rotation, given that many issues still have to be further investigated, focuses on the basics and some particular aspects while aiming to show why it is important, from a physical point of view, to study stellar rotation. Based on courses given at a graduate school, these tutorial lectures will be of interest and useful to a rather broad audience of scientists and students. 410 0$aLecture notes in physics ;$v765. 606 $aStars$xRotation 607 $aSun$xRotation 615 0$aStars$xRotation. 676 $a523.73 701 $aNeiner$b C$g(Coralie)$0515339 701 $aRozelot$b J.-P$g(Jean-Pierre),$f1942-$067603 801 0$bMiAaPQ 801 1$bMiAaPQ 801 2$bMiAaPQ 906 $aBOOK 912 $a9910143966803321 996 $aThe rotation of sun and stars$94186402 997 $aUNINA