Ivan Hubeny – författare
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5 produkter
Theory of Stellar Atmospheres
An Introduction to Astrophysical Non-equilibrium Quantitative Spectroscopic Analysis
Av Ivan Hubeny, Dimitri Mihalas
Häftad, 2014
1038 kr
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This book provides an in-depth and self-contained treatment of the latest advances achieved in quantitative spectroscopic analyses of the observable outer layers of stars and similar objects. Written by two leading researchers in the field, it presents a comprehensive account of both the physical …
Stellar Atmospheres: Beyond Classical Models
Av L. Crivellari, Ivan Hubeny m. fl.
Inbunden, 1991
2189 kr
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The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the …
From Interacting Binaries to Exoplanets (IAU S282)
Essential Modeling Tools
Av Mercedes T. Richards, Ivan Hubeny
Inbunden, 2012
1188 kr
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In IAU Symposium 282, members of the exoplanet and binary star communities unite for the first time to discuss the state-of-the-art discovery, imaging, modeling and analysis tools used to study stars, brown dwarfs and exoplanets in multiple-object systems. They describe detection techniques using …
Stellar Atmospheres: Beyond Classical Models
Av L. Crivellari, Ivan Hubeny m. fl.
Häftad, 2012
2189 kr
Lägg i varukorg
The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the …
Stellar Atmospheres: Beyond Classical Models
Av D. Hummer, Ivan Hubeny m. fl.
E-bok, 2012
2925 kr
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The theory of stellar atmospheres is one of the most important branches of modern astrophysics. It is first of all a major tool for understanding all aspects of stars. As the physical properties of their outer layers can now be found with high precision, firm conclusions can be drawn about the …
