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Physics of Thermal Gaseous Nebulae - Physical Processes in Gaseous Nebulae (Paperback, Softcover reprint of the original 1st ed. 1984)
Loot Price: R4,385
Discovery Miles 43 850
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Physics of Thermal Gaseous Nebulae - Physical Processes in Gaseous Nebulae (Paperback, Softcover reprint of the original 1st ed. 1984)
Series: Astrophysics and Space Science Library, 112
Expected to ship within 10 - 15 working days
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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.
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