Arie J. Zuckerman – författare

The knowledge and practice of clinical virology continues to expand. This new fifth edition has thirty-six comprehensive chapters, each of which has been extensively revised or rewritten, with the addition of new colour plates.

This updated version takes into account knowledge accumulated in molecular biology with its applications for laboratory diagnosis, immunisation and antiviral chemotherapy. Each chapter highlights the clinical features and epidemiological patterns of infection. Similarly, in response to the global concern of the threat posed by new viruses, a new chapter on Emerging Infections is included.  

There is also new material on Hospital Acquired Infections, including some advice relating to SARS, that will be of benefit to those dealing with the day-to-day management of patients in hospital. 

 

 

Principles and Practice of Clinical Virology is the bible for all working in the field of clinical virology – from the trainee to the expert because there’s always something new to learn! As before, the book provides a detailed account of the diagnosis and treatment of virus infections, with a stronger emphasis on clinical expertise and management. Each chapter deals with a single virus or group or viruses and is written by leading international experts in the field.

What’s new in this edition …

Showcases the wealth of new knowledge acquired on virus infections and reflects the discovery of newly recognized emerging infections, the improvement or development of new vaccines, and an increasing repertoire of antiviral agents for treatment All chapters have been thoroughly revised and there are a number of new contributors, joining the cadre of internationally-recognized experts Includes a new chapter on vaccinology covering the principles relating to the development and use of vaccines generally, which complements the specific vaccines described in the other chapters The two chapters on nosocomial infections have been enlarged and will be particularly useful for those having to advise on the management of hospital-acquired infections Emphasizes the rapid accumulation of new information in such fields as retroviruses, particularly HIV, SARS, hepatitis C and influenza, including avian influenza

The 4th edition of Viral Hepatitis covers comprehensively the entire complex field of infections caused by all of the different hepatitis viruses, which affect many millions of people throughout the world with considerable morbidity and mortality.

Howard Thomas and Arie Zuckerman are joined by Anna Lok from the USA and Stephen Locarnini from Australia as Editors.  They have recruited leading researchers and physicians from many countries, who have produced an authoritative account of current knowledge and research on this important infection, including new insights into immune response to HBV and HCV. 

The result is a comprehensive account on all aspects of viral hepatitis, including rapid advances in the diagnosis, management, treatment and prevention of a complex infection, which in the case of hepatitis B, C and D may lead to severe complications including chronic hepatitis, cirrhosis and hepatocellular carcinoma.

The latest edition of Viral Hepatitis offers an essential resource of current information for hepatologists, gastroenterologists, infectious diseases specialists and other clinicians, researchers, public health physicians and National and International Health Authorities.

The 4th edition of Viral Hepatitis covers comprehensively the entire complex field of infections caused by all of the different hepatitis viruses, which affect many millions of people throughout the world with considerable morbidity and mortality.

Howard Thomas and Arie Zuckerman are joined by Anna Lok from the USA and Stephen Locarnini from Australia as Editors.  They have recruited leading researchers and physicians from many countries, who have produced an authoritative account of current knowledge and research on this important infection, including new insights into immune response to HBV and HCV. 

The result is a comprehensive account on all aspects of viral hepatitis, including rapid advances in the diagnosis, management, treatment and prevention of a complex infection, which in the case of hepatitis B, C and D may lead to severe complications including chronic hepatitis, cirrhosis and hepatocellular carcinoma.

The latest edition of Viral Hepatitis offers an essential resource of current information for hepatologists, gastroenterologists, infectious diseases specialists and other clinicians, researchers, public health physicians and National and International Health Authorities.

This book will assemble the views of many of the world's experts in the field of viruses and diabetes. It will look critically at some unanswered questions, in the field. Among these, How do viruses destroy or modify the pancreatic islet? Which viruses are involved? What is the role of virus-induced cytokines> Could vaccines prevent virus-induced diabetes? Until recent technological advances, progress in the understanding of the relationship between viruses and diabetes has been hampered. New technologies are helping shed new light on these mysteries. This will be the first comprehensive volume on this topic.

This book will assemble the views of many of the world''s experts in the field of viruses and diabetes. It will look critically at some unanswered questions, in the field. Among these, How do viruses destroy or modify the pancreatic islet? Which viruses are involved? What is the role of virus-induced cytokines> Could vaccines prevent virus-induced diabetes? Until recent technological advances, progress in the understanding of the relationship between viruses and diabetes has been hampered. New technologies are helping shed new light on these mysteries. This will be the first comprehensive volume on this topic.

Hepatitis Viruses of Man covers the advances and developments in the study of viral hepatitis. The book discusses the history, epidemiology, and clinical features of viral hepatitis; the nomenclature and morphology of hepatitis viruses and their antigens; and the pathology of the liver in acute viral hepatitis. The text also describes the biochemical and biophysical properties of hepatitis B surface antigen; the nature and immunopathogenesis of hepatitis B; and the laboratory tests for hepatitis B surface antigen and antibody and hepatitis B core antigen and antibody. The carrier state; maternal transmission of hepatitis B and neonatal infection; and Hepatitis B virus and primary liver cancer are also considered. The book further tackles the laboratory tests for hepatitis A and the nature of the virus; immunization against hepatitis; and interferon and antiviral therapy in chronic hepatitis B infection. Microbiologists, pathologists, and medical doctors will find the book useful.

This book will assemble the views of many of the world's experts in the field of viruses and diabetes. It will look critically at some unanswered questions, in the field. Among these, How do viruses destroy or modify the pancreatic islet? Which viruses are involved? What is the role of virus-induced cytokines> Could vaccines prevent virus-induced diabetes? Until recent technological advances, progress in the understanding of the relationship between viruses and diabetes has been hampered. New technologies are helping shed new light on these mysteries. This will be the first comprehensive volume on this topic.

Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi­ gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?".

Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi­ gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?".

Red giant and supergiant stars have long been favorites of professional 6 and amateur astronomers. These enormous stars emit up to 10 times more energy than the Sun and, so, are easy to study. Some of them, specifically the pulsating long-period variables, significantly change their size, brightness, and color within about a year, a time scale of interest to a single human being. Some aspects of the study of red giant stars are similar to the study of pre-main-sequence stars. For example, optical astronomy gives us a tantalizing glimpse of star forming regions but to really investi­ gate young stars and protostars requires infrared and radio astronomy. The same is true of post-main-sequence stars that are losing mass. Optical astronomers can measure the atomic component of winds from red giant stars that are undergoing mass loss at modest rates 6 (M $ 10- M9/yr.). But to see dust grains and molecules properly, 5 especially in stars with truly large mass loss rates, ~ 10- M9/yr, one requires IR and radio astronomy. As this stage of copious mass loss only lasts for ~105 years one might be tempted to ask, "who cares?".