## Physics of the Interstellar and Intergalactic Medium

**Author**: Bruce T. Draine

**Publisher:**Princeton University Press

**ISBN:**9781400839087

**Category:**Science

**Page:**560

**View:**3512

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This is a comprehensive and richly illustrated textbook on the astrophysics of the interstellar and intergalactic medium--the gas and dust, as well as the electromagnetic radiation, cosmic rays, and magnetic and gravitational fields, present between the stars in a galaxy and also between galaxies themselves. Topics include radiative processes across the electromagnetic spectrum; radiative transfer; ionization; heating and cooling; astrochemistry; interstellar dust; fluid dynamics, including ionization fronts and shock waves; cosmic rays; distribution and evolution of the interstellar medium; and star formation. While it is assumed that the reader has a background in undergraduate-level physics, including some prior exposure to atomic and molecular physics, statistical mechanics, and electromagnetism, the first six chapters of the book include a review of the basic physics that is used in later chapters. This graduate-level textbook includes references for further reading, and serves as an invaluable resource for working astrophysicists. Essential textbook on the physics of the interstellar and intergalactic medium Based on a course taught by the author for more than twenty years at Princeton University Covers radiative processes, fluid dynamics, cosmic rays, astrochemistry, interstellar dust, and more Discusses the physical state and distribution of the ionized, atomic, and molecular phases of the interstellar medium Reviews diagnostics using emission and absorption lines Features color illustrations and detailed reference materials in appendices Instructor's manual with problems and solutions (available only to teachers)

## Radiative Processes in Astrophysics

**Author**: George B. Rybicki,Alan P. Lightman

**Publisher:**John Wiley & Sons

**ISBN:**352761818X

**Category:**Science

**Page:**400

**View:**8562

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Radiative Processes in Astrophysics: This clear, straightforward, and fundamental introduction is designed to present-from a physicist's point of view-radiation processes and their applications to astrophysical phenomena and space science. It covers such topics as radiative transfer theory, relativistic covariance and kinematics, bremsstrahlung radiation, synchrotron radiation, Compton scattering, some plasma effects, and radiative transitions in atoms. Discussion begins with first principles, physically motivating and deriving all results rather than merely presenting finished formulae. However, a reasonably good physics background (introductory quantum mechanics, intermediate electromagnetic theory, special relativity, and some statistical mechanics) is required. Much of this prerequisite material is provided by brief reviews, making the book a self-contained reference for workers in the field as well as the ideal text for senior or first-year graduate students of astronomy, astrophysics, and related physics courses. Radiative Processes in Astrophysics also contains about 75 problems, with solutions, illustrating applications of the material and methods for calculating results. This important and integral section emphasizes physical intuition by presenting important results that are used throughout the main text; it is here that most of the practical astrophysical applications become apparent.

## The Physics and Chemistry of the Interstellar Medium

**Author**: A. G. G. M. Tielens

**Publisher:**Cambridge University Press

**ISBN:**9780521826341

**Category:**Science

**Page:**495

**View:**6812

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A comprehensive overview of theoretical and observational understanding of the interstellar medium of galaxies.

## Unsolved Problems in Astrophysics

**Author**: John N. Bahcall,Jeremiah P. Ostriker

**Publisher:**Princeton University Press

**ISBN:**0691188564

**Category:**Science

**Page:**N.A

**View:**5300

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## Astrophysics of Gaseous Nebulae and Active Galactic Nuclei

**Author**: Donald E. Osterbrock,G. J. Ferland

**Publisher:**University Science Books

**ISBN:**9781891389344

**Category:**Science

**Page:**461

**View:**9732

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Thoroughly revised and expanded throughout, the new edition is a graduate-level text and reference book on gaseous nebulae, nova and supernova remnants. Much of the new data and new images are from the Hubble Space Telescope with two wholly new chapters being added along with other new features. The previous edition which was tried and tested for thirty years has now been succeeded by a revised, updated, larger edition, which will be valuable to anyone seriously interested in astrophysics.

## Physical Processes in the Interstellar Medium

**Author**: Lyman Spitzer, Jr.

**Publisher:**Wiley-VCH

**ISBN:**9780471293354

**Category:**Science

**Page:**335

**View:**4037

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Physical Processes in the Interstellar Medium discusses the nature of interstellar matter, with a strong emphasis on basic physical principles, and summarizes the present state of knowledge about the interstellar medium by providing the latest observational data. Physics and chemistry of the interstellar medium are treated, with frequent references to observational results. The overall equilibrium and dynamical state of the interstellar gas are described, with discussions of explosions produced by star birth and star death and the initial phases of cloud collapse leading to star formation.

## Astronomical Spectroscopy

*An Introduction to the Atomic and Molecular Physics of Astronomical Spectra Second Edition*

**Author**: Jonathan Tennyson

**Publisher:**World Scientific Publishing Company

**ISBN:**9813100990

**Category:**Science

**Page:**236

**View:**1467

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Nearly all information about the Universe comes from the study of light as it reaches us. However, understanding the information contained in this light requires both telescopes capable of resolving it into its component colours and a detailed knowledge of the quantum mechanical behaviour of atoms and molecules. This book, which is based on a third-year undergraduate course taught by the author at University College London, presents the basic atomic and molecular physics necessary to understand and interpret astronomical spectra. It explains how and what kind of information can be extracted from these spectra. Contemporary astronomical spectra are used extensively to study the underlying atomic physics and illustrate the results.

## Cosmological Physics

**Author**: J. A. Peacock

**Publisher:**Cambridge University Press

**ISBN:**9780521422703

**Category:**Science

**Page:**682

**View:**3097

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An eagerly-awaited, comprehensive and authoritative introduction to contemporary cosmology; for advanced undergraduate and graduate students.

## Astrophysics

*Decoding the Cosmos*

**Author**: Judith Ann Irwin

**Publisher:**John Wiley & Sons

**ISBN:**9780470319482

**Category:**Science

**Page:**446

**View:**670

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Astrophysics: Decoding the Cosmos is an accessible introduction to the key principles and theories underlying astrophysics. This text takes a close look at the radiation and particles that we receive from astronomical objects, providing a thorough understanding of what this tells us, drawing the information together using examples to illustrate the process of astrophysics. Chapters dedicated to objects showing complex processes are written in an accessible manner and pull relevant background information together to put the subject firmly into context. The intention of the author is that the book will be a ‘tool chest’ for undergraduate astronomers wanting to know the how of astrophysics. Students will gain a thorough grasp of the key principles, ensuring that this often-difficult subject becomes more accessible.

## Principles of Stellar Evolution and Nucleosynthesis

**Author**: Donald D. Clayton

**Publisher:**University of Chicago Press

**ISBN:**9780226109534

**Category:**Science

**Page:**612

**View:**1308

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Donald D. Clayton's Principles of Stellar Evolution and Nucleosynthesis remains the standard work on the subject, a popular textbook for students in astronomy and astrophysics and a rich sourcebook for researchers. The basic principles of physics as they apply to the origin and evolution of stars and physical processes of the stellar interior are thoroughly and systematically set out. Clayton's new preface, which includes commentary and selected references to the recent literature, reviews the most important research carried out since the book's original publication in 1968.

## Stellar Interiors

*Physical Principles, Structure, and Evolution*

**Author**: Carl J. Hansen,Steven D Kawaler,Virginia Trimble

**Publisher:**Springer Science & Business Media

**ISBN:**9780387200897

**Category:**Science

**Page:**526

**View:**8786

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The?rsteditionofthistextappearedin1994.Shortlyafterthethirdprinting, our editor suggested that we attempt a second edition because new devel- mentsinstellarstructureandevolutionhadmadeouroriginalworkoutdated. We (the original authors, CJH and SDK) reluctantly agreed but with res- vations due to the e?ort involved. Our initial reluctance disappeared when we were able to convince (cajole, twist the arm of, etc.) our new coauth- colleague Virginia Trimble to join us. (Welcome Virginia!) We (i.e., all three of us) hope that you agree that the present edition is a great improvement compared to the 1994 e?ort. Our objectives in this edition are the same ones we set forth in 1994: Whatyouwill?ndisatextdesignedforourtargetaudience:thety- cal senior undergraduate or beginning graduate student in astronomy or astrophysics who wishes an overview of stellar structure and e- lution with just enough detail to understand the general picture. She or he can go on from there to more specialized texts or directly to the research literature depending on talent and interests. To this end, this text presents the basic physical principles without chasing all the (interesting!) details. For those of you familiar with the ?rst edition, you will ?nd that some things have not been changed substantially (F = ma is still F = ma), while othersde?nitelyhave.Forexample,Chapter2hasbeencompletelyrewritten.

## Interstellar and Intergalactic Medium

**Author**: Barbara Ryden,Richard Pogge

**Publisher:**The Ohio State University

**ISBN:**N.A

**Category:**

**Page:**N.A

**View:**2036

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Interstellar and Intergalactic Medium is a text aimed at graduate students and advanced undergraduates in astronomy and physics; its scope is appropriate to a one-semester course. The text discusses the phases of the interstellar gas, emphasizing the role of heating, cooling, ionization, recombination, and radiative transport. The interaction between interstellar gas and dust is also discussed. In addition to the `classical' study of the interstellar medium, the rapidly developing field of circumgalactic and intergalactic gas is also included. In this text, first in the Ohio State Graduate Astrophysics Series, emphasis is placed on order-of-magnitude calculations and the development of physical insight.

## Measuring the Universe

*A Multiwavelength Perspective*

**Author**: George H. Rieke

**Publisher:**Cambridge University Press

**ISBN:**0521762294

**Category:**Science

**Page:**343

**View:**2066

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A one-stop guide to astronomical instrumentation and data acquisition, with a focus on the underlying principles behind each instrument's operation.

## Numerical Methods in Astrophysics

*An Introduction*

**Author**: Peter Bodenheimer,Gregory P. Laughlin,Michal Rozyczka,Tomasz Plewa,Harold. W Yorke,Harold W. Yorke

**Publisher:**CRC Press

**ISBN:**9780750308830

**Category:**Science

**Page:**344

**View:**2047

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Numerical Methods in Astrophysics: An Introduction outlines various fundamental numerical methods that can solve gravitational dynamics, hydrodynamics, and radiation transport equations. This resource indicates which methods are most 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. After an introduction to the basic equations and derivations, the book focuses on practical applications of the numerical methods. It explores hydrodynamic problems in one dimension, N-body particle dynamics, smoothed particle hydrodynamics, and stellar structure and evolution. The authors also examine advanced techniques in grid-based hydrodynamics, evaluate the methods for calculating the gravitational forces in an astrophysical system, and discuss specific problems in grid-based methods for radiation transfer. The book incorporates brief user instructions and a CD-ROM of the numerical codes, allowing readers to experiment with the codes to suit their own needs. With numerous examples and sample problems that cover a wide range of current research topics, this highly practical guide illustrates how to solve key astrophysics problems, providing a clear introduction for graduate and undergraduate students as well as researchers and professionals.

## Galactic Dynamics

*Second Edition*

**Author**: James Binney,Scott Tremaine

**Publisher:**Princeton University Press

**ISBN:**1400828724

**Category:**Science

**Page:**904

**View:**6306

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Since it was first published in 1987, Galactic Dynamics has become the most widely used advanced textbook on the structure and dynamics of galaxies and one of the most cited references in astrophysics. Now, in this extensively revised and updated edition, James Binney and Scott Tremaine describe the dramatic recent advances in this subject, making Galactic Dynamics the most authoritative introduction to galactic astrophysics available to advanced undergraduate students, graduate students, and researchers. Every part of the book has been thoroughly overhauled, and many sections have been completely rewritten. Many new topics are covered, including N-body simulation methods, black holes in stellar systems, linear stability and response theory, and galaxy formation in the cosmological context. Binney and Tremaine, two of the world's leading astrophysicists, use the tools of theoretical physics to describe how galaxies and other stellar systems work, succinctly and lucidly explaining theoretical principles and their applications to observational phenomena. They provide readers with an understanding of stellar dynamics at the level needed to reach the frontiers of the subject. This new edition of the classic text is the definitive introduction to the field. ? A complete revision and update of one of the most cited references in astrophysics Provides a comprehensive description of the dynamical structure and evolution of galaxies and other stellar systems Serves as both a graduate textbook and a resource for researchers Includes 20 color illustrations, 205 figures, and more than 200 problems Covers the gravitational N-body problem, hierarchical galaxy formation, galaxy mergers, dark matter, spiral structure, numerical simulations, orbits and chaos, equilibrium and stability of stellar systems, evolution of binary stars and star clusters, and much more Companion volume to Galactic Astronomy, the definitive book on the phenomenology of galaxies and star clusters

## The Chemistry of Cosmic

**Author**: David A Williams,Cesare Cecchi-Pestellini

**Publisher:**Royal Society of Chemistry

**ISBN:**1782620478

**Category:**SCIENCE

**Page:**304

**View:**7715

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This is the first book devoted to a study of the chemistry of cosmic dust, presenting current thinking on the subject distilled from many publications in surface and solid-state science, and in astronomy.

## The First Galaxies in the Universe

**Author**: Abraham Loeb,Steven R. Furlanetto

**Publisher:**Princeton University Press

**ISBN:**0691144923

**Category:**Science

**Page:**540

**View:**2856

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This book provides a comprehensive, self-contained introduction to one of the most exciting frontiers in astrophysics today: the quest to understand how the oldest and most distant galaxies in our universe first formed. Until now, most research on this question has been theoretical, but the next few years will bring about a new generation of large telescopes that promise to supply a flood of data about the infant universe during its first billion years after the big bang. This book bridges the gap between theory and observation. It is an invaluable reference for students and researchers on early galaxies. The First Galaxies in the Universe starts from basic physical principles before moving on to more advanced material. Topics include the gravitational growth of structure, the intergalactic medium, the formation and evolution of the first stars and black holes, feedback and galaxy evolution, reionization, 21-cm cosmology, and more. Provides a comprehensive introduction to this exciting frontier in astrophysics Begins from first principles Covers advanced topics such as the first stars and 21-cm cosmology Prepares students for research using the next generation of large telescopes Discusses many open questions to be explored in the coming decade

## An Introduction to the Theory of Stellar Structure and Evolution

**Author**: Dina Prialnik

**Publisher:**Cambridge University Press

**ISBN:**1316284301

**Category:**Science

**Page:**N.A

**View:**7697

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Using fundamental physics, the theory of stellar structure and evolution can predict how stars are born, how their complex internal structure changes, what nuclear fuel they burn, and their ultimate fate. This textbook is a stimulating introduction for undergraduates in astronomy, physics and applied mathematics, taking a course on the physics of stars. It uniquely emphasises the basic physical principles governing stellar structure and evolution. This second edition contains two new chapters on mass loss from stars and interacting binary stars, and new exercises. Clear and methodical, it explains the processes in simple terms, while maintaining mathematical rigour. Starting from general principles, this textbook leads students step-by-step to a global, comprehensive understanding of the subject. Fifty exercises and full solutions allow students to test their understanding. No prior knowledge of astronomy is required, and only a basic background in physics and mathematics is necessary.

## Dynamical Astrochemistry

**Author**: David A Williams,Thomas W Hartquist,Jonathan M C Rawlings,Cesare Cecchi-Pestellini,Serena Viti

**Publisher:**Royal Society of Chemistry

**ISBN:**1782627766

**Category:**Science

**Page:**290

**View:**3711

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Astrochemistry is a well-established interdisciplinary subject and the methods for describing time-dependent chemistry in static or slowly-changing regions of interstellar space have been well-developed over many years. Existing astrochemical books normally describe the subject in terms of chemistry in static or slowly-varying astronomical situations but the most significant astronomical regions are those in which the physical conditions change on timescales that are comparable to or shorter than chemical timescales. Written by leading experts in this area, this is the first book specifically devoted to the astrochemistry of dynamically evolving astronomical regions. It provides a comprehensive description of this important area of science, stressing in particular the methods that have been developed for specific purposes. It will be of interest to researchers in astrochemistry, including both chemists and physicists and could form the basis of a postgraduate course for research students in chemistry and physics.

## Essential Radio Astronomy

**Author**: James J. Condon,Scott M. Ransom

**Publisher:**Princeton University Press

**ISBN:**1400881161

**Category:**Science

**Page:**376

**View:**3185

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Essential Radio Astronomy is the only textbook on the subject specifically designed for a one-semester introductory course for advanced undergraduates or graduate students in astronomy and astrophysics. It starts from first principles in order to fill gaps in students' backgrounds, make teaching easier for professors who are not expert radio astronomers, and provide a useful reference to the essential equations used by practitioners. This unique textbook reflects the fact that students of multiwavelength astronomy typically can afford to spend only one semester studying the observational techniques particular to each wavelength band. Essential Radio Astronomy presents only the most crucial concepts—succinctly and accessibly. It covers the general principles behind radio telescopes, receivers, and digital backends without getting bogged down in engineering details. Emphasizing the physical processes in radio sources, the book's approach is shaped by the view that radio astrophysics owes more to thermodynamics than electromagnetism. Proven in the classroom and generously illustrated throughout, Essential Radio Astronomy is an invaluable resource for students and researchers alike. The only textbook specifically designed for a one-semester course in radio astronomy Starts from first principles Makes teaching easier for astronomy professors who are not expert radio astronomers Emphasizes the physical processes in radio sources Covers the principles behind radio telescopes and receivers Provides the essential equations and fundamental constants used by practitioners Supplementary website includes lecture notes, problem sets, exams, and links to interactive demonstrations An online illustration package is available to professors