Principles of Star Formation [recurso electrónico] / by Peter H. Bodenheimer.
Tipo de material: TextoSeries Astronomy and Astrophysics LibraryEditor: Berlin, Heidelberg : Springer Berlin Heidelberg, 2011Descripción: XII, 348 p. online resourceTipo de contenido: text Tipo de medio: computer Tipo de portador: online resourceISBN: 9783642150630Tema(s): Physics | Astrophysics | Physics | Astrophysics and Astroparticles | Astronomy, Observations and Techniques | Extraterrestrial Physics, Space SciencesFormatos físicos adicionales: Printed edition:: Sin títuloClasificación CDD: 523.01 Clasificación LoC:QB460-466Recursos en línea: Libro electrónicoTipo de ítem | Biblioteca actual | Colección | Signatura | Copia número | Estado | Fecha de vencimiento | Código de barras |
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Libro Electrónico | Biblioteca Electrónica | Colección de Libros Electrónicos | QB460 -466 (Browse shelf(Abre debajo)) | 1 | No para préstamo | 374934-2001 |
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.
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.
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