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The Science of Interstellar

The Science of Interstellar
Author: Kip Thorne
Publisher: W. W. Norton & Company
Total Pages: 560
Release: 2014-11-07
Genre: Science
ISBN: 0393351386

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A journey through the otherworldly science behind Christopher Nolan’s award-winning film, Interstellar, from executive producer and Nobel Prize-winning physicist Kip Thorne. Interstellar, from acclaimed filmmaker Christopher Nolan, takes us on a fantastic voyage far beyond our solar system. Yet in The Science of Interstellar, Kip Thorne, the Nobel prize-winning physicist who assisted Nolan on the scientific aspects of Interstellar, shows us that the movie’s jaw-dropping events and stunning, never-before-attempted visuals are grounded in real science. Thorne shares his experiences working as the science adviser on the film and then moves on to the science itself. In chapters on wormholes, black holes, interstellar travel, and much more, Thorne’s scientific insights—many of them triggered during the actual scripting and shooting of Interstellar—describe the physical laws that govern our universe and the truly astounding phenomena that those laws make possible. Interstellar and all related characters and elements are trademarks of and © Warner Bros. Entertainment Inc. (s14).


Physics and Chemistry of the Interstellar Medium

Physics and Chemistry of the Interstellar Medium
Author: Sun Kwok
Publisher: University Science Books
Total Pages: 594
Release: 2007-01-30
Genre: Science
ISBN: 9781891389467

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Sun Kwok explains the fundamental physics and chemistry required for understanding the interstellar medium. The textbook is interlaced with mathematical derivations that are clean, elegant and easily understandable by those with an undergraduate background in physics.


The Interstellar Medium, Expanding Nebulae and Triggered Star Formation

The Interstellar Medium, Expanding Nebulae and Triggered Star Formation
Author: Thomas G. Bisbas
Publisher: Springer
Total Pages: 82
Release: 2015-11-24
Genre: Science
ISBN: 3319261428

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This brief brings together the theoretical aspects of star formation and ionized regions with the most up-to-date simulations and observations. Beginning with the basic theory of star formation, the physics of expanding HII regions is reviewed in detail and a discussion on how a massive star can give birth to tens or hundreds of other stars follows. The theoretical description of star formation is shown in simplified and state-of-the-art numerical simulations, describing in a more clear way how feedback from massive stars can trigger star and planet formation. This is also combined with spectacular images of nebulae taken by talented amateur astronomers. The latter is very likely to stimulate the reader to observe the structure of nebulae from a different point of view, and better understand the associated star formation therein.


Physical Processes in the Interstellar Medium

Physical Processes in the Interstellar Medium
Author: Lyman Spitzer, Jr.
Publisher: John Wiley & Sons
Total Pages: 335
Release: 2008-11-20
Genre: Science
ISBN: 3527617736

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Physical Processes in the Interstellar Medium discusses the nature of interstellar matter, with a strong emphasis on basic physical principles, and summarizes the present state of knowledge about the interstellar medium by providing the latest observational data. Physics and chemistry of the interstellar medium are treated, with frequent references to observational results. The overall equilibrium and dynamical state of the interstellar gas are described, with discussions of explosions produced by star birth and star death and the initial phases of cloud collapse leading to star formation.


Exploration of the Outer Heliosphere and the Local Interstellar Medium

Exploration of the Outer Heliosphere and the Local Interstellar Medium
Author: National Research Council
Publisher: National Academies Press
Total Pages: 68
Release: 2004-11-25
Genre: Science
ISBN: 0309091861

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This report is the summary of a workshop held in May 2003 by the Space Studies Board's Committee on Solar and Space Physics to synthesize understanding of the physics of the outer heliosphere and the critical role played by the local interstellar medium (LISM) and to identify directions for the further exploration of this challenging environment.


The Physics and Chemistry of the Interstellar Medium

The Physics and Chemistry of the Interstellar Medium
Author: A. G. G. M. Tielens
Publisher: Cambridge University Press
Total Pages: 522
Release: 2005-08-25
Genre: Science
ISBN: 9781139445658

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This work provides a comprehensive overview of our theoretical and observational understanding of the interstellar medium of galaxies. With emphasis on the microscopic physical and chemical processes in space, and their influence on the macroscopic structure of the interstellar medium of galaxies, the book includes developments in this area of molecular astrophysics. The various heating, cooling, and chemical processes relevant for the rarefied gas and submicron-sized dust grains that constitute the interstellar medium are discussed in detail. This provides a firm foundation for an in-depth understanding of the ionized, neutral atomic, and molecular phases of the interstellar medium. The physical and chemical properties of large polycyclic aromatic hydrocarbon molecules and their role in the interstellar medium are highlighted, and the physics and chemistry of warm and dense photodissociation regions are discussed. This is an invaluable reference source for advanced undergraduate and graduate students, and research scientists.


Molecular Collisions in the Interstellar Medium

Molecular Collisions in the Interstellar Medium
Author: David Flower
Publisher: Cambridge University Press
Total Pages: 152
Release: 2003-12-04
Genre: Science
ISBN: 9780521545747

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In the interstellar medium - which occupies the space between the stars in galaxies - new stars are born from material that is replenished by the debris ejected by stars when they die. This book presents a detailed account of the atomic and molecular processes that give rise to the radiation we observe from the interstellar medium, knowledge that is essential to understanding star formation in our own and other galaxies. This Second Edition has been thoroughly updated and extended to cover related topics in radiation theory. It considers the chemistry of the interstellar medium, both in the present epoch and the early Universe. The book discusses the physics and chemistry of shock waves, which are produced by the jets of matter generated as a consequence of star formation. The methods for calculating rates of collisional excitation of interstellar molecules and atoms are explained, with emphasis on the quantum mechanical method. A comprehensive manual for studying collisional and radiative processes in the interstellar medium, this book will be ideal for researchers involved in calculating the rates of such processes, for those studying the interstellar medium and star formation, as well as for physical chemists specializing in collision theory or in the measurement of the rates of collision processes. Book jacket.


The Theory of Cosmic Grains

The Theory of Cosmic Grains
Author: Fred Hoyle
Publisher: Springer
Total Pages: 328
Release: 1991-10-31
Genre: Science
ISBN:

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Light scattering and absorption by small homogeneous particles can be worked-out exactly for spheres and infinite cylinders. Homogeneous particles of irregular shapes, when averaged with respect to rotation, have effects that can in general be well-approximated by reference to results for these two idealised cases. Likewise, small inhomogeneous particles have effects similar to homogeneous particles of the same average refractive index. Thus most problems can be solved to a satisfactory approximation by reference to the exact solutions for spheres and cylinders, which are fully stated here in the early part of the book. The sum of scattering and absorption, the extinction, is too large to be explained by inorganic materials, provided element abundances in the interstellar medium are not appreciably greater than solar, H 0 and NH3 being essentially excluded in the 2 general medium, otherwise very strong absorptions near 3p,m would be observed which they are not. A well-marked extinction maximum in the ultraviolet near 2200A has also not been explained satisfactorily by inorganic materials. Accurately formed graphite spheres with radii close to O.02p,m could conceivably provide an explanation of this ultraviolet feature but no convincing laboratory preparation of such spheres has ever been achieved.