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Introduction to Stellar Winds
 
 
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Introduction to Stellar Winds [Paperback]

Henny J. G. L. M. Lamers (Author), Joseph P. Cassinelli (Author)
4.0 out of 5 stars  See all reviews (1 customer review)

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Book Description

0521595657 978-0521595650 June 28, 1999 First Published
This long-awaited graduate textbook, written by two pioneers in the field, provides a comprehensive introduction to the observations, theories, and consequences of stellar winds. The rates of mass loss and the wind velocities are explained from basic physical principles. This textbook also includes chapters clearly explaining the formation and evolution of interstellar bubbles and the effects of mass loss on the evolution of high- and low-mass stars. Each topic is introduced simply to explain the basic processes and then developed to provide a solid foundation for understanding current research. This authoritative textbook is designed for advanced undergraduate and graduate students and researchers seeking an understanding of stellar winds and, more generally, supersonic flows from astrophysical objects. It is based on courses taught in Europe and the United States over the past twenty years and includes seventy problems for coursework or self-study.

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Editorial Reviews

Review

"This is an enlightening book, full of vivid physics. It fills a longstanding gap in the astrophysical literature and will stand as the foundation of the rapidly growing field of stellar winds." Professor Norbert Langer, University of Potsdam

"Stellar winds are ubiquitous, but their properties and mechanisms span an enormous range. This badly needed book by two well known researchers brings together theory and observation to provide an excellent, integrated treatment of a fascinating subject." Professor Hollis R. Johnson, Indiana University

"...for those interested in a deeper theoretical understanding of stellar winds, the book is certainly to be recommended." Meteoritics & Planetary Science

Book Description

This long-awaited and clearly written graduate textbook, by two pioneers of the field, is the first to provide a comprehensive introduction to the observations, theories and consequences of stellar winds. The rates of mass loss and the wind velocities are explained from basic physical principles. Each topic is introduced simply to explain the basic processes and the developed to provide a solid foundation for understanding current research. This lucid and authoritative textbook is designed for advanced undergraduate and graduate students and researchers. It is based on courses taught in Europe and the US over the past 20 years and includes 70 problems for coursework or self-study.

Product Details

  • Paperback: 456 pages
  • Publisher: Cambridge University Press; First Published edition (June 28, 1999)
  • Language: English
  • ISBN-10: 0521595657
  • ISBN-13: 978-0521595650
  • Product Dimensions: 9.6 x 6.7 x 1 inches
  • Shipping Weight: 1.9 pounds (View shipping rates and policies)
  • Average Customer Review: 4.0 out of 5 stars  See all reviews (1 customer review)
  • Amazon Best Sellers Rank: #2,015,695 in Books (See Top 100 in Books)

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4 of 5 people found the following review helpful:
4.0 out of 5 stars One of the best book about stellar winds, June 26, 2000
By A Customer
This review is from: Introduction to Stellar Winds (Paperback)
"Introduction to Stellar Winds" is simply one of the best book for those who need to know more about this topic. It's not just about the most massive stars, which have the strongest winds (e.g. Wolf Rayet stars), but also other stars (cooler, e.g. our Sun) with fainter wind. As a PhD student working on hot stars, this book is a reference. It sum it up all modern concepts, usually previously published in several articles in some astronomical publications. Mainly for astrophysicists, or for interested astronomy amateur whith extensive mathematical and physical knowledge.
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Inside This Book (learn more)
First Sentence:
Stellar winds are the continuous outflow of material from stars. Read the first page
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
line driven winds, polytropic winds, rotator theory, snowplow phase, dust driven winds, isothermal wind, rotator winds, rotator forces, driven wind models, condensation radius, finite disk correction, effective escape velocity, flux mean opacity, radiative acceleration, different mass loss rates, coronal winds, driven wind theory, conductive luminosity, magnetic rotator, maximum mass loss rate, solar wind theory, wave luminosity, large mass loss rates, radial momentum equation, gas momentum equation
Key Phrases - Capitalized Phrases (CAPs): (learn more)
Combining Eqs, San Francisco, Courtesy of John Mathis
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