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Stellar Atmospheres: Beyond Classical Models - L. Crivellari
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L. Crivellari:

Stellar Atmospheres: Beyond Classical Models - Paperback

2012, ISBN: 9401055742

[EAN: 9789401055741], Neubuch, [SC: 0.0], [PU: Springer Netherlands], ACCRETION; GALAXY; LOPES; QUASAR; ASTROPHYSICS; GALAXIES; INTERTTER; MAGNETOSPHERE; NEUTRONSTAR; QUASARS; UNIVERSE, D… More...

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Stellar Atmospheres: Beyond Classical Models - Crivellari, L.|Hubeny, Ivan|Hummer, D.
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Crivellari, L.|Hubeny, Ivan|Hummer, D.:

Stellar Atmospheres: Beyond Classical Models - Paperback

2012, ISBN: 9401055742

[EAN: 9789401055741], Neubuch, [PU: Springer Netherlands], ACCRETION GALAXY LOPES QUASAR ASTROPHYSICS GALAXIES INTERTTER MAGNETOSPHERE NEUTRONSTAR QUASARS UNIVERSE PHYSIK ASTRONOMIE INTER… More...

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Stellar Atmospheres: Beyond Classical Models - Crivellari, L. Hubeny, Ivan Hummer, D.
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Crivellari, L. Hubeny, Ivan Hummer, D.:
Stellar Atmospheres: Beyond Classical Models - First edition

2012

ISBN: 9789401055741

Paperback

[ED: Kartoniert / Broschiert], [PU: Springer Netherlands], Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. Proceedings of the NATO Advance… More...

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Stellar Atmospheres: Beyond Classical Models - Crivellari, L. (Herausgeber); Hummer, D. (Herausgeber); Hubeny, Ivan (Herausgeber)
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Crivellari, L. (Herausgeber); Hummer, D. (Herausgeber); Hubeny, Ivan (Herausgeber):
Stellar Atmospheres: Beyond Classical Models - Paperback

2012, ISBN: 9401055742

Softcover reprint of the original 1st ed. 1991 Kartoniert / Broschiert Accretion; galaxy; LOPES; Quasar; astrophysics; galaxies; intertter; magnetosphere; NeutronStar; quasars; Universe… More...

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Stellar Atmospheres: Beyond Classical Models - L. Crivellari; Ivan Hubeny; D. Hummer
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L. Crivellari; Ivan Hubeny; D. Hummer:
Stellar Atmospheres: Beyond Classical Models - Paperback

2012, ISBN: 9789401055741

Buch, Softcover, Softcover reprint of the original 1st ed. 1991, [PU: Springer], Springer, 2012

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Details of the book
Stellar Atmospheres: Beyond Classical Models
Author:
Title:
ISBN:

9401055742

Details of the book - Stellar Atmospheres: Beyond Classical Models


EAN (ISBN-13): 9789401055741
ISBN (ISBN-10): 9401055742
Paperback
Publishing year: 2014
Publisher: Springer

Book in our database since 2014-09-26T12:01:15-04:00 (New York)
Detail page last modified on 2022-09-23T12:53:02-04:00 (New York)
ISBN/EAN: 9401055742

ISBN - alternate spelling:
94-010-5574-2, 978-94-010-5574-1
Alternate spelling and related search-keywords:
Book author: hubeny
Book title: stellar atmospheres, stella mode

Information from Publisher

Author: L. Crivellari; Ivan Hubeny; D. Hummer
Title: Nato Science Series C:; Stellar Atmospheres: Beyond Classical Models
Publisher: Springer; Springer Netherland
461 Pages
Publishing year: 2012-10-23
Dordrecht; NL
Printed / Made in
Language: English
213,99 € (DE)
219,99 € (AT)
236,00 CHF (CH)
POD
XIV, 461 p.

BC; Hardcover, Softcover / Physik, Astronomie/Astronomie; Astrophysik; Verstehen; Accretion; Galaxy; LOPES; Quasar; astrophysics; galaxies; interstellar matter; magnetosphere; neutron star; quasars; stellar; universe; Astrophysics; BB; EA

Section 1..- Recent Advances in Computational Methods.- Acceleration of Convergence.- Fast Solution of Radiative Transfer Problems with a Multi-Grid Method.- Line Blanketing without LTE: Simple and Complex Spectra.- Global and Local Methods for 1-D Problems; Implementation Aspects and CPU-Time and Memory Scalings.- 2-D Axisymmetric Line Transport.- NLTE Spectral Line Formation in Three Dimensions.- Iteration with Approximate Lambda Operators, and its Application to the Expanding Atmospheres of WR Stars.- Analytical Methods of Line Formation Theory: Are They Still Alive?.- Iteration Factors in the Solution of the NLTE Line Transfer Problem.- Analysis of Ultraviolet P Cygni Profiles in the Spectra of O-Type Stars.- Computer Codes for Stellar Atmospheric Modeling.- Section 2..- The Quest for Physical Realism in Stellar Atmospheric Modeling.- Unified NLTE Model Atmospheres Including Spherical Extension and Stellar Winds: Euv-Fluxes and the HE II Discrepancy in Central Stars of Planetary Nebulae.- Non-LTE Model Atmosphere Calculations with Approximate Lambda Operators.- NLTE Model Atmospheres for Hot Stars.- Radiative Transfer in Expanding Atmospheres - Radiative Acceleration of Wolf-Rayet Envelopes?.- Non-LTE Analysis of Hot Stars Including Line Blanketing.- Time-Dependent Two-Dimensional Radiation Hydrodynamics of Accreting Matter onto Highly Magnetized Neutron Stars: The Evolution of Photon Bubbles.- The Origin and Development of Instabilities in Radiatively- Driven Stellar Winds.- A Smooth Source Function Method for Including Scattering in Radiatively Driven Wind Simulations.- 2-D Radiation Hydrodynamics Models of the Solar Photosphere.- Dynamics of and Radiative Transfer in Inhomogeneous Media.- Atmospheres of Late-Type Giants.- Fe II Emission Line Diagnostics of the Sun and Stars.- Chromospheric Inhomogeneities in Cool Stars: Possible Effect on Hydrogen Line Profiles.- Numerical Simulation of Photospheric Convection: Hydrodynamical Test Calculations.- Section 3..- Stellar Atmosphere Theory as a Spectroscopic Tool. The Example of Hot Stars.- The Winds of O-Stars. V: Tests of the Accuracy of the Radiation Driven Wind Models.- Diagnostics of Wolf-Rayet Atmospheres.- Central Stars of PN: Spectral Diagnostics Based on Model Atmospheres VS. Diagnostics Based on the Classical Nebular Approach.- Spectral Diagnostics of Hot Subdwarfs: Successes and Problems.- Temperatures, Gravities and Abundances of B Stars: Recent Progress and Remaining Problems.- Line Blanketing Without LTE: The Effect on Diagnostics for B-Type Stars.- Particle Transport in Magnetic Stellar Atmospheres.- Spectroscopic Tests of Late-Type Model Atmospheres of Dwarf Stars.- Dust in the Shells of Cool Giants and Supergiants.- NLTE Analysis of Massive OB Stars.- Formation of the K I 7699 Å Line in Sunspots.- On the Influence of Multi-Dimensional Radiative Transfer on the Energetic Contribution of the Ca K Line.- Special Session.- The Opacity Project and the Practical Utilization of Atomic Data.- New Opacity Calculations.- 40 Years Numerical Stellar Atmospheres: Concluding Remarks and Personal Considerations.

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