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Frank and Joe Hardy have been sent on a mission to live on the edge! A new theme park, Galaxy X, is about to open. But someone out there obviously wants Galaxy X to go away. The park owner has received threatening e-mails, and accidents are becoming frequent. In Galaxy X, the brothers have to find the saboteur before opening day, or someone could get seriously hurt. In X-plosion, Frank and Joe must trail pro skater Cody Zane, brought to Galaxy X for the grand opening, and find out who would want to end his career just as it’s about to explode. . . .
Frank and Joe Hardy have been sent on a mission to live on the edge! A new theme park, Galaxy X, is about to open. But someone out there obviously wants Galaxy X to go away. The park owner has received threatening e-mails, and accidents are becoming frequent. In Galaxy X, the brothers have to find the saboteur before opening day, or someone could get seriously hurt. In X-plosion, Frank and Joe must trail pro skater Cody Zane, brought to Galaxy X for the grand opening, and find out who would want to end his career just as it’s about to explode. . . .
The Black Vortex, an ancient artifact imbued with immeasurable power, is now in the hands of Mr. Knife! With billions of lives potentially at stake, Peter Quill, the Legendary Star-Lord, is going to have to dust off his thieving gloves. But with Knife's Slaughter Squad protecting him, Peter's probably going to need some help...Collecting: Guardians of the Galaxy & X-Men: The Black Vortex Alpha #1, Guardians of the Galaxy (2014) #24-25, Legendary Star-Lord (2014) #9-11, All-New X-Men #38-39, Guardians Team-Up #2, Nova #28, Cyclops (2014) #12, Captain Marvel (2014) #14, Guardians of the Galaxy & X-Men: The Black Vortex Omega #1
2020 IBPA Awards Winner! "I honestly can't recommend this book enough" Starwarsnews.net "This book takes things to a whole new, and massive, level. Magnificent to behold" Geekdad.com From famed New York Times best-selling paper engineer Matthew Reinhart comes Star Wars: The Ultimate Pop-Up Galaxy. This glorious pop-up book is a fitting tribute to the entire Star Wars saga, from A New Hope to The Rise Of Skywalker See Padmé battle alongside the Jedi and clone troopers, Luke train with Jedi Master Yoda on Dagobah, and Rey and Kylo Ren battle Supreme Leader Snoke’s Praetorian Guards, as well as other memorable moments from the saga. With five amazing scenes rich with detail and secrets that fold out into one breathtaking map of the entire Star Wars saga, Star Wars: The Ultimate Pop-Up Galaxy is the perfect gift for boys, girls, and Star Wars fans of all ages. —The Entire Star Wars Saga. Featuring all 11 Star Wars movies, including A New Hope, Rogue One, Revenge of the Sith, and The Rise Of Skywalker. —Illustrious Characters. Jedi, Sith, royalty, and rogues are all featured. See Han Solo, Princess Leia, Chewbacca, Finn, Poe Dameron, Mace Windu, Darth Sidious, General Hux, Supreme Leader Snoke, and more! —Legendary Locations. See locations come to life, including Geonosis, Mustafar, Yavin, Tatooine, Crait, Endor, and, of course, the notorious Death Star and the fearsome Starkiller Base. —Iconic Moments. Witness battles and duels from across the saga, including the Jedi’s heroic struggle on Geonosis, the battle of Hoth, Obi-Wan Kenobi’s tragic duel with Anakin Skywalker, and Anakin’s rebirth as the fearsome Darth Vader. —Famous Vehicles. See the Millennium Falcon, Star Destroyers, X-wings, TIE fighters, snowspeeders, AT-ATs, and other vehicles from the saga.
Galaxies, along with their underlying dark matter halos, constitute the building blocks of structure in the Universe. Of all fundamental forces, gravity is the dominant one that drives the evolution of structures from small density seeds at early times to the galaxies we see today. The interactions among myriads of stars, or dark matter particles, in a gravitating structure produce a system with fascinating connotations to thermodynamics, with some analogies and some fundamental differences. Ignacio Ferreras presents a concise introduction to extragalactic astrophysics, with emphasis on stellar dynamics, and the growth of density fluctuations in an expanding Universe. Additional chapters are devoted to smaller systems (stellar clusters) and larger ones (galaxy clusters). Fundamentals of Galaxy Dynamics, Formation and Evolution is written for advanced undergraduates and beginning postgraduate students, providing a useful tool to get up to speed in a starting research career. Some of the derivations for the most important results are presented in detail to enable students appreciate the beauty of maths as a tool to understand the workings of galaxies. Each chapter includes a set of problems to help the student advance with the material.
First published in 1988, this book is a comprehensive survey of the astrophysical characteristics of the hot gas which pervades clusters of galaxies. In our universe, clusters of galaxies are the largest organised structures. Typically they comprise hundreds of galaxies moving through a region of space ten million light years in diameter. The volume between the galaxies is filled with gas having a temperature of 100 million degrees. This material is a strong source of cosmic X-rays. Dr Sarazin describes the theoretical description of the origin, dynamics, and physical state of the cluster gas. Observations by radio and optical telescopes are also summarised. This account is addressed to professional astronomers and to graduate students. It is an exhaustive summary of a rapidly expanding field of research in modern astrophysics.
In the year 2299, seventh-grader Jack and his classmates find themselves in hostile alien territory after Jack accidentally launches their rickety public schoolship light years away from home.
This classic text - aimed at senior undergraduates and beginning graduate students in physics and astronomy - presents a wide range of concepts in sufficient depth to give the reader a quantitative understanding of the subject. Emphasising physical concepts, it provides the student with a series of astrophysical sketches, concluding with a synthesis of all the subjects discussed in the book, sketching the history of the universe from its beginning to the formation of the Sun and the planets.
This is a book about physics, written for mathematicians. The readers we have in mind can be roughly described as those who: I. are mathematics graduate students with some knowledge of global differential geometry 2. have had the equivalent of freshman physics, and find popular accounts of astrophysics and cosmology interesting 3. appreciate mathematical elarity, but are willing to accept physical motiva tions for the mathematics in place of mathematical ones 4. are willing to spend time and effort mastering certain technical details, such as those in Section 1. 1. Each book disappoints so me readers. This one will disappoint: 1. physicists who want to use this book as a first course on differential geometry 2. mathematicians who think Lorentzian manifolds are wholly similar to Riemannian ones, or that, given a sufficiently good mathematical back ground, the essentials of a subject !ike cosmology can be learned without so me hard work on boring detaiis 3. those who believe vague philosophical arguments have more than historical and heuristic significance, that general relativity should somehow be "proved," or that axiomatization of this subject is useful 4. those who want an encyclopedic treatment (the books by Hawking-Ellis [1], Penrose [1], Weinberg [1], and Misner-Thorne-Wheeler [I] go further into the subject than we do; see also the survey article, Sachs-Wu [1]). 5. mathematicians who want to learn quantum physics or unified fieId theory (unfortunateIy, quantum physics texts all seem either to be for physicists, or merely concerned with formaI mathematics).
Mergers are the mechanisms by which galaxy clusters are assembled through the hierarchical growth of smaller clusters and groups. Major cluster mergers are the most energetic events in the Universe since the Big Bang. Many of the observed properties of clusters depend on the physics of the merging process. These include substructure, shock, intra cluster plasma temperature and entropy structure, mixing of heavy elements within the intra cluster medium, acceleration of high-energy particles, formation of radio halos and the effects on the galaxy radio emission. This book reviews our current understanding of cluster merging from an observational and theoretical perspective, and is appropriate for both graduate students and researchers in the field.