The origin and evolution of planetary nebulae / Sun Kwok.
Material type:
TextSeries: Cambridge astrophysics series ; 33.Publisher: Cambridge : Cambridge University Press, 2000Description: 1 online resource (xiii, 243 pages) : digital, PDF file(s)Content type: - text
- computer
- online resource
- 9780511529504 (ebook)
- The Origin & Evolution of Planetary Nebulae
- 523.1/135 21
- QB855.5 .K96 2000
Title from publisher's bibliographic system (viewed on 05 Oct 2015).
History and overview -- Ionization structure of planetary nebulae -- Nebular line radiation -- Nebular continuum radiation -- The neutral gas component -- The dust component -- Observation of the cental star of planetary nebulae -- Morphologies of planetary nebulae -- Problems and questions -- Asymptotic giant branch stars -- progenitors of planetary nebulae -- Evolution of the central stars -- Formation of planetary nebulae -- Dynamical evolution of planetary nebulae -- Protoplanetary nebulae -- the transition objects -- Evolution to the white dwarf stage -- Distances to planetary nebulae -- Comparison between evolutionary models and observations -- PN in the galactic context -- Nebulae in other galaxies -- Concluding remarks.
This authoritative volume provides a comprehensive review of the origin and evolution of planetary nebulae. It covers all the stages of their evolution, carefully synthesizes observations from across the spectrum, and clearly explains all the key physical processes at work. Particular emphasis is placed on observations from space, using the Hubble Space Telescope, the Infrared Space Observatory, and the ROSAT satellite. This book presents a thoroughly modern understanding of planetary nebulae, integrating developments in stellar physics with the dynamics of nebular evolution. It also describes exciting possibilities such as the use of planetary nebulae in determining the cosmic distance scale, the distribution of dark matter and the chemical evolution of galaxies. This book provides graduate students with an accessible introduction to planetary nebulae, and researchers with an authoritative reference. It can also be used as an advanced text on the physics of the interstellar medium.
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