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The Physics and Dynamics of Planetary Nebulae (Astronomy and Astrophysics Library)
 
 
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The Physics and Dynamics of Planetary Nebulae (Astronomy and Astrophysics Library) [Hardcover]

Grigor A. Gurzadyan (Author)
5.0 out of 5 stars  See all reviews (1 customer review)

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Book Description

3540609652 978-3540609650 May 16, 1997 1
This is a considerably revised English translation of the Russian original of 1993. It gives a rather complete survey of the astrophysics of planetary nebulae, including theory and observations. The book covers various subjects ranging from various aspects of emission lines, ionization equilibrium, electron temperature, the ultraviolet and the continuous spectra, the infrared radiation and radio emission all the way to distances, dimensions, dynamics and, finally, the origin of planetary nebulae. It addresses students as well as professional and amateur astronomers.

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Language Notes

Text: English (translation)
Original Language: Russian

From the Back Cover

The physics and dynamics of planetary nebulae are surveyed in this comprehensive monograph. The topics covered include processes occurring in the highly ionized gaseous medium, the formation of emission lines in rather specific conditions, continuous emissions extending from radio frequencies and infrared up to ultraviolet and X-rays, and methods of deciphering the observed spectra and detecting the physical and kinematic parameters of the radiating medium. Many of these methods have become powerful tools for the study of various other cosmic objects from stellar atmospheres to galactic nuclei. Special attention is paid to discoveries made using space observations. The problems of the origin of planetary nebulae and their evolution are discussed extensively. A catalogue of planetary nebulae by excitation classes is also included. The book should remain a standard reference for students and researchers in the field for years to come.

Product Details

  • Hardcover: 529 pages
  • Publisher: Springer; 1 edition (May 16, 1997)
  • Language: English
  • ISBN-10: 3540609652
  • ISBN-13: 978-3540609650
  • Product Dimensions: 9.6 x 6.3 x 1 inches
  • Shipping Weight: 2 pounds (View shipping rates and policies)
  • Average Customer Review: 5.0 out of 5 stars  See all reviews (1 customer review)
  • Amazon Best Sellers Rank: #4,508,331 in Books (See Top 100 in Books)

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2 of 2 people found the following review helpful:
5.0 out of 5 stars Excellent book for professional work on planetary nebulae, April 24, 2009
This review is from: The Physics and Dynamics of Planetary Nebulae (Astronomy and Astrophysics Library) (Hardcover)
English could be better (certainly the translation from russian) but despite the detailed and complex maths around planetary nebulae physics, this book provides an excellent insight on how it works. I found some precious data and explanation there. Professional level or for amateur with high level of maths/physics background.
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Inside This Book (learn more)
First Sentence:
Planetary nebulae are expanding gaseous envelopes of enormous size in the centre of which the so-called nucleus of the nebula a high temperature star, the source of the excitation of the nebula's light emission is located. Read the first page
Key Phrases - Statistically Improbable Phrases (SIPs): (learn more)
decrement diagram, high excitation nebulae, low excitation nebulae, excitation class, helium nebulae, infrared forbidden lines, optically thick nebulae, optically thin nebula, dynamical separation, given nebula, ionization formula, former nuclei, nebula increases, nova envelopes, volume emission coefficient, neutral envelope, infrared emission lines, nebular conditions, nucleus temperature, individual nebulae, interstellar extinction, dilution coefficient, nuclei temperatures, expanding nebula, lust particles
Key Phrases - Capitalized Phrases (CAPs): (learn more)
Rayleigh Taylor, Hubble Space Telescope, Magellanic Clouds, Mira Ceti, Nova Aquila, Small Magellanic Cloud, Theoretical Continuous Spectra of Nebulae, New Class of Nebulae
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