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Principles of Star Formation Peter H. Bodenheimer Buch Book Englisch 2011 - edition reliée, livre de poche

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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. 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. Both theoretical and observational evidence to support the validity of the general evolutionary path are presented, and methods for comparing the two are emphasized. The author is a recognized expert in calculations of the evolution of protostars, the structure and evolution of disks, and stellar evolution in general. This book will be of value to graduate students in astronomy and astrophysics as well as to active researchers in the field.

Informations détaillées sur le livre - Principles of Star Formation


EAN (ISBN-13): 9783642150623
ISBN (ISBN-10): 3642150624
Version reliée
Date de parution: 2011
Editeur: Springer Berlin
380 Pages
Poids: 0,678 kg
Langue: Englisch

Livre dans la base de données depuis 2009-06-30T04:51:46+02:00 (Paris)
Page de détail modifiée en dernier sur 2022-11-15T14:37:11+01:00 (Paris)
ISBN/EAN: 9783642150623

ISBN - Autres types d'écriture:
3-642-15062-4, 978-3-642-15062-3
Autres types d'écriture et termes associés:
Auteur du livre: bodenheimer, peter bode, bodenheim
Titre du livre: bodenheimer, astronomy and astrophysics


Données de l'éditeur

Auteur: Peter Bodenheimer
Titre: Astronomy and Astrophysics Library; Principles of Star Formation
Editeur: Springer; Springer Berlin
348 Pages
Date de parution: 2011-07-10
Berlin; Heidelberg; DE
Imprimé / Fabriqué en
Langue: Anglais
106,99 € (DE)
109,99 € (AT)
118,00 CHF (CH)
POD
XII, 348 p.

BB; Hardcover, Softcover / Physik, Astronomie/Astronomie; Astrophysik; Verstehen; Astronomie, Kartographie; Formation of First Stars; Massive Star Formation; Molecular Clouds; Pre-main-sequence evolution; Protostar Collapse; Protostellar Disks; Star Cluster Formation; Star Formation Accretion; Star Formation in the Early Universe; Star Formation, Gravitational Collapse; Star Formation, Infrared Observations; Star Formation, Radio Observations; Star Formation, graduate textbook; Star forming regions; Stellar Initial Mass Function; Stellar Winds and Outflows; Young Stars; Astrophysics; Astronomy, Observations and Techniques; Space Physics; Astronomische Beobachtung: Observatorien, Ausrüstungen und Methoden; Angewandte Physik; Sonnensystem: Sonne und Planeten; BC

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 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. Both theoretical and observational evidence to support the validity of the general evolutionary path are presented, and methods for comparing the two are emphasized. The author is a recognized expert in calculations of the evolution of protostars, the structure and evolution of disks, and stellar evolution in general. This book will be of value to graduate students in astronomy and astrophysics as well as to active researchers in the field.

Overview.- Molecular Clouds and the Onset of Star Formation.- Protostar Collapse.- Rotating Protostars and Accretion Disks.- Massive Star Formation.- Formation of Binary Systems.- The Formation of the First Stars.- Pre-main-sequence Evolution.- Summary: Issues in Galactic Star Formation.- References.- Index.

From the reviews:

“This is an absolutely superb book, from the beginning of the preface, where the author provides a basic definition of star formation, to the last section where he reminds us that ‘efficiency’ of star formation can mean at least three different things, with three different numerical value … . The 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 be obtained.” (Virginia Trimble, The Observatory, Vol. 132 (1226), February, 2012)

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 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. Both theoretical and observational evidence to support the validity of the general evolutionary path are presented, and methods for comparing the two are emphasized. The author is a recognized expert in calculations of the evolution of protostars, the structure and evolution of disks, and stellar evolution in general. This book will be of value to graduate students in astronomy and astrophysics as well as to active researchers in the field.


Most up-to-date graduate text on a key field in astrophysics Covers a wide variety of physical processes necessary to understand star formation With detailed discussion of key points in star formation Compares theoretical models of star formation with observational evidence Author is an internationally recognized expert in calculating the evolution of protostars and stellar evolution Includes supplementary material: sn.pub/extras

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