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Stellar Atmospheres: Theory and Observations Lectures Held at the Astrophysics School IX, Organized by the European Astrophysics Doctoral Network (EADN) in Brussels, Belgium, 10-19 September 1996.

The 1996 Summer School of the European Astrophysical Doctoral Network dealt with the atmospheres of stars, the various theories that describe their structure and the interactions with the interior of the stars as well as with the interstellar environment, and the observations that support, modify an...

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Bibliographic Details
Other Authors: Greve, Jean P.de (Editor), Blomme, Ronny (Editor), Hensberge, Herman (Editor)
Format: eBook
Language:English
Published: Berlin, Heidelberg Springer Berlin Heidelberg 1997, 1997
Edition:1st ed. 1997
Series:Lecture Notes in Physics
Subjects:
Astronomy / Observations
Astronomy, Observations And Techniques
Astrophysics
Online Access:
Collection: Springer Book Archives -2004 - Collection details see MPG.ReNa
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245 0 0 |a Stellar Atmospheres: Theory and Observations  |h Elektronische Ressource  |b Lectures Held at the Astrophysics School IX, Organized by the European Astrophysics Doctoral Network (EADN) in Brussels, Belgium, 10-19 September 1996.  |c edited by Jean P.de Greve, Ronny Blomme, Herman Hensberge 
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505 0 |a Stellar atmospheres theory: An introduction -- Stellar wind theories -- Cool star winds and mass loss: Theory -- Cool stars winds and mass loss: Observations -- The theory of line driven stellar winds -- Observations of hot-star winds -- Circumstellar disks -- Stellar coronae -- Atmospheres and interior models 
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653 |a Astrophysics 
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700 1 |a Hensberge, Herman  |e [editor] 
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520 |a The 1996 Summer School of the European Astrophysical Doctoral Network dealt with the atmospheres of stars, the various theories that describe their structure and the interactions with the interior of the stars as well as with the interstellar environment, and the observations that support, modify and sometimes contradict these theories. This volume aims to provide the reader with an insight into problems related to stellar atmospheres both for cool and for hot stars. Furthermore it offers opportunities to deal with modern technologies in analysing observational data versus theoretical modelling 

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