Accretion discs are ubiquitous in astrophysics. It occurs around strong magnetic stars in X-ray binary pulsars, magnetic white dwarfs, in cataclysmic variables, and T Taurus stars, etc.The interaction between a magnetized; rotating star and a surrounding accretion disc has been of continued interest since the discovery of X-ray pulsars in binary systems. In spite of the early progress, interaction of the accretion disc with in the stellar magnetosphere is not yet well understood. The subject of this book will therefore be to construct a theoretical model which can be used as the basis for further analytical and numerical investigations for accretion disc around magnetized stars including effect of the magnetic field generated by an internal dynamo. I believe that this book will give a good background of X-ray binaries, X-ray pulsars and magnetic field interactions and application of MHD equations in accretion disc theory. The book is mainly used for graduate students, Post doc and senior researchers and will act as a basis for subsequent investigations accretion discs around magnetised stars.
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Solomon Belay Tessema(PhD)was receieved Bsc. degree in Physics and Msc. in Astrophysics. In 2010 he has been received his PhD in Astrophysics from Addis Ababa University undersupervision of Ulf Torkelsson University of Gotherburg, Sweden. Currently he is lecturer and researcher at Kotebe College department of Physics at rank of Assistant Professor
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Taschenbuch. Zustand: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -Accretion discs are ubiquitous in astrophysics. It occurs around strong magnetic stars in X-ray binary pulsars, magnetic white dwarfs, in cataclysmic variables, and T Taurus stars, etc.The interaction between a magnetized; rotating star and a surrounding accretion disc has been of continued interest since the discovery of X-ray pulsars in binary systems. In spite of the early progress, interaction of the accretion disc with in the stellar magnetosphere is not yet well understood. The subject of this book will therefore be to construct a theoretical model which can be used as the basis for further analytical and numerical investigations for accretion disc around magnetized stars including effect of the magnetic field generated by an internal dynamo. I believe that this book will give a good background of X-ray binaries, X-ray pulsars and magnetic field interactions and application of MHD equations in accretion disc theory. The book is mainly used for graduate students, Post doc and senior researchers and will act as a basis for subsequent investigations accretion discs around magnetised stars. 132 pp. Englisch. Bestandsnummer des Verkäufers 9783845417363
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Zustand: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Tessema Solomon BelaySolomon Belay Tessema(PhD)was receieved Bsc. degree in Physics and Msc. in Astrophysics. In 2010 he has been received his PhD in Astrophysics from Addis Ababa University undersupervision of Ulf Torkelsson Univers. Bestandsnummer des Verkäufers 5481461
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Taschenbuch. Zustand: Neu. This item is printed on demand - Print on Demand Titel. Neuware -Accretion discs are ubiquitous in astrophysics. It occurs around strong magneticstars in X-ray binary pulsars, magnetic white dwarfs, in cataclysmic variables,and T Taurus stars, etc.The interaction between a magnetized; rotating star anda surrounding accretion disc has been of continued interest since the discoveryof X-ray pulsars in binary systems. In spite of the early progress, interaction ofthe accretion disc with in the stellar magnetosphere is not yet well understood.The subject of this book will therefore be to construct a theoretical model whichcan be used as the basis for further analytical and numerical investigations foraccretion disc around magnetized stars including effect of the magnetic fieldgenerated by an internal dynamo. I believe that this book will give a goodbackground of X-ray binaries, X-ray pulsars and magnetic field interactions andapplication of MHD equations in accretion disc theory. The book is mainly usedfor graduate students, Post doc and senior researchers and will act as a basis forsubsequent investigations accretion discs around magnetised stars.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 132 pp. Englisch. Bestandsnummer des Verkäufers 9783845417363
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Taschenbuch. Zustand: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - Accretion discs are ubiquitous in astrophysics. It occurs around strong magnetic stars in X-ray binary pulsars, magnetic white dwarfs, in cataclysmic variables, and T Taurus stars, etc.The interaction between a magnetized; rotating star and a surrounding accretion disc has been of continued interest since the discovery of X-ray pulsars in binary systems. In spite of the early progress, interaction of the accretion disc with in the stellar magnetosphere is not yet well understood. The subject of this book will therefore be to construct a theoretical model which can be used as the basis for further analytical and numerical investigations for accretion disc around magnetized stars including effect of the magnetic field generated by an internal dynamo. I believe that this book will give a good background of X-ray binaries, X-ray pulsars and magnetic field interactions and application of MHD equations in accretion disc theory. The book is mainly used for graduate students, Post doc and senior researchers and will act as a basis for subsequent investigations accretion discs around magnetised stars. Bestandsnummer des Verkäufers 9783845417363
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Taschenbuch. Zustand: Neu. ACCRETION DISCS AROUND MAGNETIZED STARS, IN PARTICULAR NEUTRON STARS | Accretion discs around magnetized stars | Solomon Belay Tessema | Taschenbuch | 132 S. | Englisch | 2011 | LAP LAMBERT Academic Publishing | EAN 9783845417363 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu. Bestandsnummer des Verkäufers 106883935
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