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Cosmic inflation and dark energy hold the key to the origin and the eventual fate of the Universe. Despite the increasing prominence of these subjects in research and teaching over the past decade or more, no introductory text dedicated to this topic has been previously published.

This book, the first of two volumes, is the first undergraduate-level textbook exclusively devoted to radio astronomy telescopes and observation methods. It explains the instrumentation and techniques needed to make successful observations in radio astronomy. Requiring no prior knowledge of astronomy, the text prepares students to contribute to

Written by a specialist in stellar astrophysics, this book presents a rigorous but accessible treatment of the physics of stellar explosions from a multidisciplinary perspective at the crossroads of computational astrophysics, observational astronomy, cosmochemistry, and nuclear physics. Basic concepts from all these different fields are applied

Written by an award-winnning cosmologist, this new textbook provides advanced undergraduate and graduate students with coverage of the very latest developments in the field. Problems and solutions are included and more advanced extension material is offered in the Appendix, ensuring the book is accessible to students.

Written by one of the world's leading cosmologists, this brand-new, thoroughly class-tested textbook provides graduate and undergraduate students with coverage of the very latest developments and experimental results in the field. Prof. Nicola Vittorio shows what is meant by precision cosmology, from both theoretical and observational perspectiv

This book discusses cosmology from both an observational and a strong theoretical perspective. Readers will gain a comprehensive account of cosmology and the latest observational results, without requiring prior knowledge of relativistic theories, making the text ideal for students.

Cosmic inflation and dark energy hold the key to the origin and the eventual fate of the Universe. Despite the increasing prominence of these subjects in research and teaching over the past decade or more, no introductory text dedicated to this topic has been previously published.

Describes historical (pre-1950) theories about solar system and illustrates why they became unacceptable. This book also critically examines extant theories, including the solar nebula theory, to determine how well they fit with accepted scientific principles and observations.

Interstellar dust clouds catalyze simple chemical reactions, absorb, scatter, polarize, and re-radiate starlight, and form the building blocks for planet and stellar formation. This book provides a theoretical description of the fundamental physics of interstellar material, including a description of its composition, morphology, and grain size.

Offers an introduction to modern ideas on the physical basis of the theory of relativity. This book explores various theories and ideas in big bang cosmology, providing an insight into problems. It presents the standard big bang theory of the universe and also provides an introduction to inflationary cosmology, emphasizing the underlying physics.

Beginning from the physical background of spectroscopy with an explanation of energy levels and spectroscopic notation, this book introduces the main techniques of optical spectroscopy and the range of instrumentation. It describes the applications of spectroscopy in modern astronomy, such as the solar system, stars, nebulae, and galaxies.

This two-volume set of introductory textbooks are the first exclusively devoted to radio astronomy, and the telescopes, observation methods, and astrophysical processes that furnish this exciting field. The set enables instructors to pick and choose topics from the two volumes that best fit their courses.

This undergraduate textbook presents an extensive introduction to the astrophysical processes that enable radio astronomy. It discusses the physical phenomena that give rise to radio emissions, presenting examples of astronomical objects, and illustrating how the physical parameters of astronomical sources can be obtained from radio observations.

This book discusses cosmology from both an observational and a strong theoretical perspective. Readers will gain a comprehensive account of cosmology and the latest observational results, without requiring prior knowledge of relativistic theories, making the text ideal for students.

Written by one of the world's leading cosmologists, this brand-new, thoroughly class-tested textbook provides graduate and undergraduate students with coverage of the very latest developments and experimental results in the field. Prof. Nicola Vittorio shows what is meant by precision cosmology, from both theoretical and observational perspectives.

Offering practical advice on a range of wavelengths and tools, this highly accessible, self-contained book presents a broad overview of astronomical instrumentation, techniques, and tools.

Written by a specialist in stellar astrophysics, this book presents a rigorous but accessible treatment of the physics of stellar explosions from a multidisciplinary perspective at the crossroads of computational astrophysics, observational astronomy, cosmochemistry, and nuclear physics. Basic concepts from all these different fields are applied to the study of classical and recurrent novae, type I and II supernovae, X-ray bursts and superbursts, and stellar mergers. The book shows how a multidisciplinary approach has been instrumental in our understanding of nucleosynthesis in stars.

This book, the first of two volumes, is the first undergraduate-level textbook exclusively devoted to radio astronomy telescopes and observation methods. It explains the instrumentation and techniques needed to make successful observations in radio astronomy. Requiring no prior knowledge of astronomy, the text prepares students to contribute to a radio astronomy research team. It includes examples throughout and end-of-chapter problems as well as lab exercises on the book¿s CRC Press web page.

Answers the questions of 'why is the night sky dark' and 'just how dark is it' both qualitatively and quantitatively from the viewpoints of both history and modern cosmology. This title compares the observational data from telescopes with the cosmological theory based on general relativity and particle physics.

Dust is widespread in the galaxy. To astronomers studying stars it may be just an irritating fog, but it is becoming widely recognized that cosmic dust plays an active role in astrochemistry. This book covers the role of dust in the formation of molecules in the interstellar medium, with the exception of dust in the solar system.

Outlines various fundamental numerical methods that solve gravitational dynamics, hydrodynamics, and radiation transport equations. This book shows which methods are suitable for particular problems, demonstrates what the accuracy requirements are in numerical simulations, and suggests ways to test for and reduce the inevitable negative effects.