An Introduction To The Theory Of Stellar Structure And Evolution

Autor: Dina Prialnik
Publisher: Cambridge University Press
ISBN: 1316284301
File Size: 42,59 MB
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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.

An Introduction To The Theory Of Stellar Structure And Evolution

Autor: Dina Prialnik
Publisher: Cambridge University Press
ISBN: 1316284301
File Size: 18,94 MB
Format: PDF, ePub, Docs
Read: 2363
Download or Read Book
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.

Astrophysics Through Computation

Autor: Brian Koberlein
Publisher: Cambridge University Press
ISBN: 1107010748
File Size: 63,24 MB
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This new astrophysics text integrates analytical and computational methods to explore a broad range of topics in astrophysics.

Stellar Structure And Evolution

Autor: Rudolf Kippenhahn
Publisher: Springer Science & Business Media
ISBN: 3642615236
File Size: 52,29 MB
Format: PDF, Docs
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A complete and comprehensive treatment of the physics of the stellar interior and the underlying fundamental processes and parameters. The text presents an overview of the models developed to explain the stability, dynamics and evolution of the stars, and great care is taken to detail the various stages in a star's life. The authors have succeeded in producing a unique text based on their own pioneering work in stellar modeling. Since its publication, this textbook has come to be considered a classic by both readers and teachers in astrophysics. This study edition is intended for students in astronomy and physics alike.

Cosmological Physics

Autor: J. A. Peacock
Publisher: Cambridge University Press
ISBN: 9780521422703
File Size: 12,80 MB
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An eagerly-awaited, comprehensive and authoritative introduction to contemporary cosmology; for advanced undergraduate and graduate students.

An Introduction To The Sun And Stars

Autor: Simon F. Green
Publisher: Cambridge University Press
ISBN: 9780521546225
File Size: 48,47 MB
Format: PDF
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Compiled by a team of experts, this textbook has been designed for elementary university courses in astronomy and astrophysics. It starts with a detailed discussion of our nearest star, the Sun, and describes how solar physicists have come to understand its internal workings. It then considers how astronomers go about studying the basic physical properties and life-cycles of more distant stars, and culminates with a discussion of the formation of exotic objects such as neutron stars and black holes. Written in an accessible style that avoids complex mathematics, and illustrated in colour throughout, this book is suitable for self-study and will appeal to amateur astronomers as well as undergraduate students. It contains numerous helpful learning features such as boxed summaries, student exercises with full solutions, and a glossary of terms. The book is also supported by a website hosting further teaching materials.

Blood Profits

Autor: Vanessa Neumann
Publisher: St. Martin's Press
ISBN: 1250089360
File Size: 79,66 MB
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International smuggling has exploded, deepening and accelerating the collaboration of transnational organized crime and terrorist groups. Attacks like the Charlie Hebdo and Bataclan shootings in Paris, the kidnappings and murders by Boko Haram in Nigeria, and the San Bernardino shooting were partially funded by seemingly harmless illegal goods such as cheap cigarettes, smuggled oil, prostitution, fake Viagra, fake designer bags, and even bootleg DVDs. But how can this be? In Blood Profits, Vanessa Neumann, an expert on dismantling illicit trade, explains how purchasing illegal goods translates to supporting organized crime and terrorists. Neumann shows how the effects of the collapsed Iron Curtain, USSR scientists and intelligence agents left without work, regional trade pacts, the dissipation of the East-versus-West mentality, and new-age technology have all led to an intricate network of illegal trade. She leads the reader through a variety of cases, both by geography and by industry (selecting industries where illicit trade is generally poorly understood), before extracting lessons learned into some policy recommendations that we can all embrace.

The Stars

Autor: Roger John Tayler
Publisher: Cambridge University Press
ISBN: 9780521458856
File Size: 58,12 MB
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This textbook gives a clear account of the manner in which knowledge in many branches of physics, such as gravitation, thermodynamics, atomic physics, and nuclear physics, can be combined to gain an understanding of the structure and evolution of stars. A major aim is to present the subject as one in which advances are still being made. The first half is an account of the observational properties of stars and a discussion of the equations that govern their structure. The second part discusses recent theoretical work on stellar evolution. The successes of the theory are stressed, but attention is also drawn to phenomena that are not completely understood. This is a new edition of a widely-used textbook first published in 1970. New topics include mass loss from stars and close binary stars.

Stellar Interiors

Autor: Carl J. Hansen
Publisher: Springer Science & Business Media
ISBN: 9780387200897
File Size: 66,20 MB
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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.