Principles of star formation by Peter Bodenheimer

Cover of: Principles of star formation | Peter Bodenheimer

Published by Springer in Berlin, New York .

Written in English

Read online

Subjects:

  • Evolution,
  • Formation,
  • Stars

Edition Notes

Includes bibliographical references (p. 325-338) and index.

Book details

StatementPeter H. Bodenheimer
SeriesAstronomy and astrophysics library, Astronomy and astrophysics library
Classifications
LC ClassificationsQB806 .B63 2011
The Physical Object
Paginationxi, 343 p. :
Number of Pages343
ID Numbers
Open LibraryOL25058863M
ISBN 103642150624
ISBN 109783642150623
LC Control Number2011933131
OCLC/WorldCa679937277

Download Principles of star formation

The current star formation in our galaxy is emphasized, because the most detailed observations are available for this case. The book presents a comparison of the various scenarios for star formation, discusses the basic physics underlying each one, and follows in detail the history of a star from its initial state in the interstellar gas to its becoming a condensed object in by: Book Title Principles of Star Formation Authors.

Peter Bodenheimer; Series Title Astronomy and Astrophysics Library Copyright Publisher Springer-Verlag Berlin Heidelberg Copyright Holder Springer-Verlag Berlin Heidelberg eBook ISBN DOI / Hardcover ISBN Softcover ISBN Series ISSN Brand: Springer-Verlag Berlin Heidelberg.

Introduction. Understanding star formation is one of the key fields in present-day astrophysics. This book treats a wide variety of the physical processes involved, as well as the main observational discoveries, with key points being discussed in detail.

The current star formation in our galaxy is emphasized, because the most detailed observations are available for this case. The current star formation in our galaxy is emphasized, because the most detailed observations are available for this case. The book presents a comparison of the various scenarios for star formation, discusses the basic physics underlying each one, and follows in detail the history of a star from its initial state in the interstellar gas to its becoming a condensed object in equilibrium.

Principles of Star Formation Understanding star formation is one of the key fields in present-day astrophysics. This book treats a wide variety of the physical processes involved, as well as the main observational discoveries, with key points being discussed in detail.

Principles of star formation. [Peter Bodenheimer] -- Understanding star formation is one of the key fields in present-day astrophysics. This book treats a wide variety of the physical processes involved, as well as the main observational discoveries.

As an introduction to the science of star formation, this book concentrates on the interpretation of observations in star-forming regions relatively nearby, in our own Galaxy, at the present time, where the most detailed and accurate results can.

"Star formation is one of the most active research fields in modern astronomy and is also the key to understanding problems as diverse as galaxy evolution and the origin of planets. This book, written by two highly regarded experts, first poses the questions that define the field of star formation and then gives a remarkably comprehensive yet concise survey of the underlying s: 4.

Understanding star formation is one of the key fields in present-day astrophysics. This book treats a wide variety of the physical processes involved, as Principles of star formation book as the main observational discoveries Author: Peter Bodenheimer.

The current star formation in our galaxy is emphasized, because the most detailed observations are available for this case. The book presents a comparison of Principles of star formation book various scenarios for star formation, discusses the basic physics underlying each one, and follows in detail the history of a star from its initial state in the interstellar gas to its becoming a condensed object in : Peter Bodenheimer.

This book, written by two highly regarded experts, first poses the questions that define the field of star formation and then gives a remarkably comprehensive yet concise survey of the underlying physics. The book provides both an overview suitable for those new to the field and also a convenient handbook for established s: 4.

adshelp[at] The ADS is operated by the Smithsonian Astrophysical Observatory under NASA Cooperative Agreement NNX16AC86ACited by: Principles of Star Formation, Peter H. Bodenheimer, Springer, New York, $ ( pp.). ISBN Buy at Amazon How starsform out of diffuse interstellar matter is a fundamental problem of astrophysicsand one that has witnessed remarkable progress over the past few decades.

• The star formation rates is determined using many different indicators. • The most important of are – far infrared emission tracing deeply embedded star formation –Hα emission tracing H II regions; –and far ultraviolet emission tracing young, massive stars that have dispersed their natal gas and dust.

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A cloud of hydrogen gas must be compressed to a sufficiently small size so that gravity dominates. (As an example, the sun is a stable sphere of gas.).

The physics of star formation forming stars, may be chaotic and create a large dispersion in the properties of stars and stellar systems. Thus, star formation processes, like most natural phenomena, probably involve a combination of regularity and randomness.

Some outcomes of star formation processes that are particularly important to. Nearly forty years ago, as he thought about the dramatic new millimeter wavelength observations of gas in star-forming molecular clouds and their newly derived masses and motions, Gary Larson realized a few basic principles seemed to be at work.

Larger clouds showed a wider range of motions, the motions implied that the kinetic energies were roughly balanced (in equilibrium) with the. This important book describes the basic principles of astrochemistry - an interdisciplinary field combining astronomy, physics, and chemistry - with particular emphasis on its physical and chemical background.

Chemical processes in diffuse clouds, dense quiescent molecular clouds, star-forming regions, and protoplanetary disks are discussed. A brief introduction to molecular spectroscopy and. This book provides a modern introduction to the study of star formation, at a level suitable for graduate students or advanced undergraduates in astrophysics.

The first third of the book provides a review of the observational phenomenology and then the basic physical processes that are important for star formation. Particularly the star formation process in present-day galaxies follows the typical principles of self-organization phenomena.

A galaxy may be considered to be an open nonequilibrium system with nonlinear process dynamics. It thus exhibits typical coherent behavior of galactic scale by long range star formation waves travelling across its.

Star formation happens when part of a dust cloud begins to contract under its own gravitational force; as it collapses, the center becomes hotter and hotter until nuclear fusion begins in the core.

That is a basic and simple summary of this chapter. Star formation begins in massive clouds of molecular gas and dust. This book is a comprehensive treatment of star formation, one of the most active fields of modern astronomy.

The reader is guided through the subject in a logically compelling manner. Starting from a general description of stars and interstellar clouds, the. This important book describes the basic principles of astrochemistry—an interdisciplinary field combining astronomy, physics, and chemistry—with particular emphasis on its physical and chemical background.

Chemical processes in diffuse clouds, dense quiescent molecular clouds, star-forming regions, and protoplanetary disks are discussed. This book is a comprehensive treatment of star formation, one of the most active fields of modern astronomy.

The reader is guided through the subject in a logically compelling manner. Starting from a general description of stars and interstellar clouds, the /5(1).

There are two main models of star formation. Gravitational collapse is a top-down process in which molecular clumps that are hundreds of times heavier than the Sun fragment into gaseous cores, which then collapse to make individual stars.

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