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Añadir al carritoCondición: New. pp. 144.
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Añadir al carritoKartoniert / Broschiert. Condición: New. The major limitation of cancer treatment is normal tissuetolerance. When irradiating normal tissue, such as the normal braintissue, one of the principal causes of complications is damage tothe cerebral vasculature. If radiation is to benefit patients, itwou.
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Añadir al carritoTaschenbuch. Condición: Neu. Radiotherapy and the Human Brain | Towards a Better Understanding of Response | Ciprian D. Igna | Taschenbuch | Kartoniert / Broschiert | Englisch | 2008 | VDM Verlag Dr. Müller | EAN 9783639046762 | Verantwortliche Person für die EU: OmniScriptum GmbH & Co. KG, Bahnhofstr. 28, 66111 Saarbrücken, info[at]akademikerverlag[dot]de | Anbieter: preigu.
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Publicado por LAP LAMBERT Academic Publishing, 2012
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Añadir al carritoTaschenbuch. Condición: Neu. The Nature and Origin of Hercules X-1's Light-curve Dips | A continuing debate | Ciprian D. Igna (u. a.) | Taschenbuch | 296 S. | Englisch | 2012 | LAP LAMBERT Academic Publishing | EAN 9783659148866 | Verantwortliche Person für die EU: preigu GmbH & Co. KG, Lengericher Landstr. 19, 49078 Osnabrück, mail[at]preigu[dot]de | Anbieter: preigu.
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Publicado por VDM Verlag Dr. Mueller Aktiengesellschaft & Co. KG, 2008
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Añadir al carritoCondición: New. Print on Demand pp. 144 23:B&W 6 x 9 in or 229 x 152 mm Perfect Bound on White w/Gloss Lam.
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Publicado por LAP LAMBERT Academic Publishing Jul 2012, 2012
ISBN 10: 3659148865 ISBN 13: 9783659148866
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Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -HZ Her/Her X-1 is one of the most popular low-mass X-ray binary star systems, which consists of a neutron star (Her X-1) and a post-main-sequence star (HZ Her). Her X-1 is one of the first two founding members of the accretion-powered X-ray pulsars class. Due to its large luminosity and low interstellar absorption Her X-1 remains one of the most studied pulsars. The system is characterized by a great wealth of phenomena including 1.24 s regular X-ray pulsations, 1.7-day orbital period eclipses, a superorbital X-ray intensity cycle of ~35 days, and a large number of highly variable X-ray absorption events coined light-curve dips by Riccardo Giacconi, one of the 2002 Physics Nobel Prize laureates and founder of X-ray Astronomy. Unlike the periodic X-ray flux modulations, the light-curve dips are not well understood despite more than 30 years of intense research work. We present here the largest and most recent record of Her X-1 s light-curve dips, and propose a theoretical model that reproduces the timing of any of the observed light-curve dips. The model is based on a single dip production mechanism and explains most dip properties, including the famous marching dip effect. 296 pp. Englisch.
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Publicado por VDM Verlag Dr. Mueller Aktiengesellschaft & Co. KG, 2008
ISBN 10: 3639046765 ISBN 13: 9783639046762
Librería: Biblios, Frankfurt am main, HESSE, Alemania
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Añadir al carritoCondición: New. PRINT ON DEMAND pp. 144.
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Publicado por LAP LAMBERT Academic Publishing, 2012
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Añadir al carritoCondición: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Autor/Autorin: Igna Ciprian D.Dr. Igna obtained his PhD at the University of Calgary. His research interests cover a wide range, including NMR coupling phenomena, Radiotherapy, Imaging and X-ray binaries. Prof. Leahy received his PhD at the Univers.
Librería: AHA-BUCH GmbH, Einbeck, Alemania
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Añadir al carritoTaschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - The major limitation of cancer treatment is normal tissuetolerance. When irradiating normal tissue, such as the normal braintissue, one of the principal causes of complications is damage tothe cerebral vasculature. If radiation is to benefit patients, itwould be beneficial to know or be able to predict the consequencesof irradiating the normal tissue. While there is some data relatingloss of perfusion to radiation dose in other tissues such as lung,there is very little data for the brain. This book describes andanalyzes the feasibility of an original method developed by theauthor in collaboration with the staff at the University ofCalgary, Tom Baker Cancer Centre and Foothills Hospital in Calgary,Canada to investigate the relationship between the change inhemodynamic measures and the radiation dose delivered to the normalbrain tissue following a typical brain tumour radiotherapyprocedure. A generous amount of space has been dedicated toexplaining some elementary concepts, since the book brings togetherinformation characteristic to various different fields, likePhysics, Medical Diagnostic Imaging and Cancer Treatment.
Idioma: Inglés
Publicado por LAP LAMBERT Academic Publishing Jul 2012, 2012
ISBN 10: 3659148865 ISBN 13: 9783659148866
Librería: buchversandmimpf2000, Emtmannsberg, BAYE, Alemania
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Añadir al carritoTaschenbuch. Condición: Neu. This item is printed on demand - Print on Demand Titel. Neuware -HZ Her/Her X-1 is one of the most popular low-mass X-ray binary star systems, which consists of a neutron star (Her X-1) and a post-main-sequence star (HZ Her). Her X-1 is one of the first two founding members of the accretion-powered X-ray pulsars class. Due to its large luminosity and low interstellar absorption Her X-1 remains one of the most studied pulsars. The system is characterized by a great wealth of phenomena including 1.24 s regular X-ray pulsations, 1.7-day orbital period eclipses, a superorbital X-ray intensity cycle of ~35 days, and a large number of highly variable X-ray absorption events coined light-curve dips by Riccardo Giacconi, one of the 2002 Physics Nobel Prize laureates and founder of X-ray Astronomy. Unlike the periodic X-ray flux modulations, the light-curve dips are not well understood despite more than 30 years of intense research work. We present here the largest and most recent record of Her X-1's light-curve dips, and propose a theoretical model that reproduces the timing of any of the observed light-curve dips. The model is based on a single dip production mechanism and explains most dip properties, including the famous marching dip effect.VDM Verlag, Dudweiler Landstraße 99, 66123 Saarbrücken 296 pp. Englisch.
Idioma: Inglés
Publicado por LAP LAMBERT Academic Publishing, 2012
ISBN 10: 3659148865 ISBN 13: 9783659148866
Librería: AHA-BUCH GmbH, Einbeck, Alemania
EUR 79,00
Cantidad disponible: 1 disponibles
Añadir al carritoTaschenbuch. Condición: Neu. nach der Bestellung gedruckt Neuware - Printed after ordering - HZ Her/Her X-1 is one of the most popular low-mass X-ray binary star systems, which consists of a neutron star (Her X-1) and a post-main-sequence star (HZ Her). Her X-1 is one of the first two founding members of the accretion-powered X-ray pulsars class. Due to its large luminosity and low interstellar absorption Her X-1 remains one of the most studied pulsars. The system is characterized by a great wealth of phenomena including 1.24 s regular X-ray pulsations, 1.7-day orbital period eclipses, a superorbital X-ray intensity cycle of ~35 days, and a large number of highly variable X-ray absorption events coined light-curve dips by Riccardo Giacconi, one of the 2002 Physics Nobel Prize laureates and founder of X-ray Astronomy. Unlike the periodic X-ray flux modulations, the light-curve dips are not well understood despite more than 30 years of intense research work. We present here the largest and most recent record of Her X-1 s light-curve dips, and propose a theoretical model that reproduces the timing of any of the observed light-curve dips. The model is based on a single dip production mechanism and explains most dip properties, including the famous marching dip effect.