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Theory Of Stellar Atmospheres An Introduction To Astrophysical Nonequilibrium Quantitative Spectroscopic Analysis Ivan Huben Dimitri Mihalas

  • SKU: BELL-10849694
Theory Of Stellar Atmospheres An Introduction To Astrophysical Nonequilibrium Quantitative Spectroscopic Analysis Ivan Huben Dimitri Mihalas
$ 31.00 $ 45.00 (-31%)

4.7

56 reviews

Theory Of Stellar Atmospheres An Introduction To Astrophysical Nonequilibrium Quantitative Spectroscopic Analysis Ivan Huben Dimitri Mihalas instant download after payment.

Publisher: Princeton University Press
File Extension: PDF
File size: 12.58 MB
Pages: 923
Author: Ivan Hubený; Dimitri Mihalas
ISBN: 9780691163284, 0691163286
Language: English
Year: 2015

Product desciption

Theory Of Stellar Atmospheres An Introduction To Astrophysical Nonequilibrium Quantitative Spectroscopic Analysis Ivan Huben Dimitri Mihalas by Ivan Hubený; Dimitri Mihalas 9780691163284, 0691163286 instant download after payment.

"This eagerly anticipated book is an excellent guide for anyone interested in radiation transport in astrophysics, as well as for those wanting to make detailed analyses of astrophysical spectra. Comprehensive, lucid, and stimulating, "Theory of Stellar Atmospheres" is ideal for students and scientists alike."--Bengt Gustafsson, Uppsala University ""Theory of Stellar Atmospheres" will become 'The Book' in this field, supplanting all others. Every serious student and researcher in astrophysics should own a copy. Hubeny and Mihalas constitute the dream team for this subject, having worked in the area for their entire careers and made fundamental and important contributions."--James M. Stone, Princeton University ""Theory of Stellar Atmospheres" is the standard by which other books in the field will be judged."--Don Winget, University of Texas at Austin "This is an impressive book. Hubeny and Mihalas review the statistical mechanics of matter and radiation; the absorption, emission, and scattering of radiation; and line broadening in the context of the non-equilibrium structure of a stellar atmosphere. They summarize the early fundamental work in the field, and give a detailed account of the methods needed to calculate and study stellar spectra."--Eugene H. Avrett, Harvard-Smithsonian Center for Astrophysics

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