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Author: Lawrence H. Aller Publisher: Cambridge University Press ISBN: 9780521310406 Category : Science Languages : en Pages : 388
Book Description
A semi-popular account of stars and gaseous nebulae, treating topics such as stellar evolution, the origin of elements, supernovae and cosmic rays.
Author: Lawrence H. Aller Publisher: Cambridge University Press ISBN: 9780521310406 Category : Science Languages : en Pages : 388
Book Description
A semi-popular account of stars and gaseous nebulae, treating topics such as stellar evolution, the origin of elements, supernovae and cosmic rays.
Author: C.R. Kitchin Publisher: CRC Press ISBN: 9780852745809 Category : Science Languages : en Pages : 386
Book Description
Stars, Nebulae and the Interstellar Medium: Observational Physics and Astrophysics complements the author's highly successful Astrophysical Techniques, Fourth Edition (2004). This book describes those characteristics of stars, groups of stars, and the material between the stars that can be directly observed or inferred from the study of electromagnetic emissions and, occasionally, high-energy particles. Providing a wealth of material of interest and use to a wide range of readers, the descriptive chapters are accessible to scientifically literate nonspecialists while the complete text is suitable for most advanced undergraduates in astrophysics.
Author: Britannica Educational Publishing Publisher: Britannica Educational Publishing ISBN: 1615300538 Category : Juvenile Nonfiction Languages : en Pages : 219
Book Description
The Sun is merely one of some 200 billion stars that make up the Milky Way--and the Milky Way is only one of a billion galaxies in the known universe. Packed with fascinating facts and stunning photography, this book examines the Galaxy humans call home and travels light years away, to the domain of phenomena such as the Oort cloud.
Author: L.H. Aller Publisher: Springer Science & Business Media ISBN: 9401096392 Category : Science Languages : en Pages : 358
Book Description
Gaseous nebulae offer outstanding opportunities to atomic physicists, spectroscopists, plasma experts, and to observers and theoreticians alike for the study of attenuated ionized gases. These nebulae are often dusty, heated by radiation fields and by shocks. They are short-lived phenomena on the scale of a stellar lifetime, but their chemical compositions and internal kinematics may give important clues to advanced stages of stellar evolution. The material herein presented is based on lectures given at the University of Michigan, University of Queensland, University of California, Los Angeles, and in more abbreviated form at the Raman Institute, at the Scuola Internazionale di Trieste, and elsewhere. Much of it is derived origionally from the series "Physical Processes in Gaseous Nebulae" initiated at the Harvard College Observatory in the late 1930s. I have tried to emphasize the basic physics of the mechanisms involved and mention some of the uncertainties that underlie calculations of many basic parameters. Emphasis is placed on ionized plasmas with electron temperatures typically in the neighborhood of 10,OOOoK. Dust and other ingredients of the cold component of the interstellar medium are treated briefly from the point of view of their relation to hot plasmas of H II regions and planetaries. Chemical composition determinations for nebulae are discussed in some detail while the last section deals with interpretations of elemental abundances in the framework of stellar evolution and nucleogenesis. Gaseous nebulae offer some particularly engaging opportunities for studies of stellar evolution.
Author: Lawrence H. Aller
Author: Lawrence H. Aller
Author: Lawrence Hugh Aller
Author: Leo Goldberg
Author: Leo Goldberg
Author: Stanley Barber Brown
Author: Sir Arthur Stanley Eddington
Author: C.R. Kitchin
Author: Beverly T. Lynds
Author: Britannica Educational Publishing
Author: L.H. Aller