Isbn: 9783540644484 - computational methods for astrohphysical fluid flow: saas-fee advanced course 27. lecture notes 1997 swiss society for astrophysics and astronomy (15 risultati)

Hardcover. Condizione: Fine. 1st Edition. EXCELLENT Unmarked PAGES And COVER. And Strong BINDING. Hardback. As Shown. No dust Jacket, as issued. Published/printed by Springer. First printing, 1998. Not ex-library or facsimile reprint. Physics Professor signature on blank end paper.

Hardcover. Condizione: Very Good. Book has light rubbing and smudging to covers with light surface scratches to back, light bends to outer bottom corners, light scuffs to tips of outer corners of front cover, a subtle bend to front endpage, faint aging to edges of pages. otherwise in very good condition, strong binding, clean and unmarked pages; some cosmetic wear but an overall sturdy reading copy.…

Condizione: New.

Condizione: Good. This is an ex-library book and may have the usual library/used-book markings inside.This book has hardback covers. In good all round condition. No dust jacket. Please note the Image in this listing is a stock photo and may not match the covers of the actual item,950grams, ISBN:9783540644484. …

Condizione: New. In.

hardcover. Condizione: New. In shrink wrap. Looks like an interesting title.

Condizione: New. pp. xiv + 508 1st Edition.

Hardcover. Condizione: Brand New. 1st edition. 508 pages. 9.50x6.50x1.00 inches. In Stock.

Buch. Condizione: Neu. Druck auf Anfrage Neuware - Printed after ordering - This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. TOC:Nonlinear Conservation Laws and Finite Volume Methods.- Radition Hydrodynamics.- Radiation Hydrodynamics: Numerical Aspects and Applications.- Simulation of Astrophysical Fluid Flow.…

Hardcover. Condizione: Like New. LIKE NEW. SHIPS FROM MULTIPLE LOCATIONS. book.

Buch. Condizione: Neu. This item is printed on demand - it takes 3-4 days longer - Neuware -This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures. TOC:Nonlinear Conservation Laws and Finite Volume Methods.- Radition Hydrodynamics.- Radiation Hydrodynamics: Numerical Aspects and Applications.- Simulation of Astrophysical Fluid Flow. 524 pp. Englisch.…

Condizione: New. Dieser Artikel ist ein Print on Demand Artikel und wird nach Ihrer Bestellung fuer Sie gedruckt. This book can be used also as a textbook for scientific modelling in fluid mechanics and astrophysicsThis book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applicat.…

Condizione: New. Print on Demand pp. xiv + 508.

Buch. Condizione: Neu. This item is printed on demand - Print on Demand Titel. Neuware -This book leads directly to the most modern numerical techniques for compressible fluid flow, with special consideration given to astrophysical applications. Emphasis is put on high-resolution shock-capturing finite-volume schemes based on Riemann solvers. The applications of such schemes, in particular the PPM method, are given and include large-scale simulations of supernova explosions by core collapse and thermonuclear burning and astrophysical jets. Parts two and three treat radiation hydrodynamics. The power of adaptive (moving) grids is demonstrated with a number of stellar-physical simulations showing very crispy shock-front structures.Springer-Verlag KG, Sachsenplatz 4-6, 1201 Wien 524 pp. Englisch.…

Condizione: New. PRINT ON DEMAND pp. xiv + 508.