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Indulge in this collection of the best astronomy books from the past 800 years. The Astronomers' Library is a rich history of astronomy (and astrology) publishing across Europe. This is a carefully selected arrangement of publications from all over the continent – Germany, France, Italy, Netherlands, Spain, and the UK. And of course, as the original world leader in astrology, the middle east is featured, with multiple books from Persia. Humankind has looked to the heavens since the dawn of time, wondering what is out there, as well as how everything works and (originally) who was responsible for it. Every tribe, race and civilization has wondered about our place in the universe and what lies beyond and what lies within it, below our feet. Lately, attention has turned to the origins of the universe. From the turn of the millennium, knowledge and ideas were recorded, first on tablets or rock, then in the form of simple manuscripts, and eventually in a much more elaborate fashion as illustrative and engraving skills evolved. The advent of printed books saw the production of highly illustrated tomes that showed off the skills of the printers as well as the newfound knowledge of the scholars and artists that wrote them. Many of these works pushed the boundaries of illustrated publishing (and continue to do so to this day). They commanded expert illustrators and skilled engravers and hence didn’t come cheaply. They were treasured in the libraries of the wealthy and their intrinsic worth has meant that there is an incredible wealth of beautifully preserved historic examples from the 14th century onwards. The significant difference we acknowledge today between astronomy and astrology has a relatively recent past, and the stars have long been associated with creatures, gods, characters and all sorts of divine beings. The study of such has a long, fascinating history that is shown in beautiful detail in the pages of these many beautiful books, and the transition from seeing the stars as characters to understanding them as spinning, celestial beings and part of our huge universe is akin to witnessing the history of the world. As far back as the tenth century, Persian scholars such as Abd al-Rahman al-Sufi was recording his findings, observations and speculations on the wider universe, in his Book of Fixed Stars. The focus turned to Europe in the Middle Ages, with Germany, Holland and England the centres of study and publication. Following the “Copernican Revolution”, observation and study underwent a radical change, paving the way for astronomers such as Kepler, Galilei and Newton to shed further light on the nature of the planets and stars of our known systems, and the ground beneath our feet. Each of those famous names contribute to the illustrated books that are featured within.
Describing interstellar matter in our galaxy in all of its various forms, this book also considers the physical and chemical processes that are occurring within this matter. The first seven chapters present the various components making up the interstellar matter and detail the ways that we are able to study them. The following seven chapters are devoted to the physical, chemical and dynamical processes that control the behaviour of interstellar matter. These include the instabilities and cloud collapse processes that lead to the formation of stars. The last chapter summarizes the transformations that can occur between the different phases of the interstellar medium. Emphasizing methods over results, The Interstellar Medium is written for graduate students, for young astronomers, and also for any researchers who have developed an interest in the interstellar medium.
With information and scale as central themes, this comprehensive survey explains how to handle real problems in astronomical data analysis using a modern arsenal of powerful techniques. It treats those innovative methods of image, signal, and data processing that are proving to be both effective and widely relevant. The authors are leaders in this rapidly developing field and draw upon decades of experience. They have been playing leading roles in international projects such as the Virtual Observatory and the Grid. The book addresses not only students and professional astronomers and astrophysicists, but also serious amateur astronomers and specialists in earth observation, medical imaging, and data mining. The coverage includes chapters or appendices on: detection and filtering; image compression; multichannel, multiscale, and catalog data analytical methods; wavelets transforms, Picard iteration, and software tools. This second edition of Starck and Murtagh's highly appreciated reference again deals with topics that are at or beyond the state of the art. It presents material which is more algorithmically oriented than most alternatives and broaches new areas like ridgelet and curvelet transforms. Throughout the book various additions and updates have been made.
High-energy astrophysics has unveiled a Universe very different from that only known from optical observations. It has revealed many types of objects in which typical variability timescales are as short as years, months, days, and hours (in quasars, X-ray binaries, etc), and even down to milli-seconds in gamma ray bursts. The sources of energy that are encountered are only very seldom nuclear fusion, and most of the time gravitation, a paradox when one thinks that gravitation is, by many orders of magnitude, the weakest of the fundamental interactions. The understanding of these objects' physical conditions and the processes revealed by high-energy astrophysics in the last decades is nowadays part of astrophysicists' culture, even of those active in other domains of astronomy. This book evolved from lectures given to master and PhD students at the University of Geneva since the early 1990s. It aims at providing astronomers and physicists intending to be active in high-energy astrophysics a broad basis on which they should be able to build the more specific knowledge they will need. While in the first part of the book the physical processes are described and derived in detail, the second part studies astrophysical objects in which high-energy astrophysics processes are crucial. This two-pronged approach will help students recognise physical processes by their observational signatures in contexts that may differ widely from those presented here.
Hardcover reprint of the original 1786 edition - beautifully bound in brown cloth covers featuring titles stamped in gold, 8vo - 6x9. No adjustments have been made to the original text, giving readers the full antiquarian experience. For quality purposes, all text and images are printed as black and white. This item is printed on demand. Book Information: Herschel, W.. Catalogue Of One Thousand New Nebulae And Clusters Of Stars. By William Herschel, Ll.D. F. R. S. Indiana: Repressed Publishing LLC, 2012. Original Publishing: Herschel, W.. Catalogue Of One Thousand New Nebulae And Clusters Of Stars. By William Herschel, Ll.D. F. R. S, . Royal Society Of London, 1786. Subject: Proceedings of the Royal Society of London
It is rare for a complete biography of an Australian scientist, particularly of an Australian woman scientist, to be published. It is rarer for such a book to be co-authored by an American. Although scientists have written discourses on the history of their discipline, it is most unusual for a scientist to write a full length biography of a colleague in his ?eld. It is also uncommon for a man to write about an Australian woman scientist; most of the work on Australian women scientists has been done by other women. However, these authors, both distinguished researchers in the ?eld of radio astr- omy, became so interested in the history of their discipline and in the career of the pioneer radio astronomer Ruby Payne-Scott that they spent some years bringing this book to fruition. Until relatively recently, Ruby Payne-Scott had been the only woman scientist mentioned brie?y in histories of Australian science or of Australian radio astronomy. This book will be an invaluable resource for anyone interested in these disciplines. Being scientists themselves, the authors explain Payne-Scott’s scienti?c work in detail; therefore, the value and importance of her contributions can, for the ?rst time, be recognised, not only by historians but also by scientists.
Targeting advanced students of astronomy and physics, as well as astronomers and physicists contemplating research on supernovae or related fields, David Branch and J. Craig Wheeler offer a modern account of the nature, causes and consequences of supernovae, as well as of issues that remain to be resolved. Owing especially to (1) the appearance of supernova 1987A in the nearby Large Magellanic Cloud, (2) the spectacularly successful use of supernovae as distance indicators for cosmology, (3) the association of some supernovae with the enigmatic cosmic gamma-ray bursts, and (4) the discovery of a class of superluminous supernovae, the pace of supernova research has been increasing sharply. This monograph serves as a broad survey of modern supernova research and a guide to the current literature. The book’s emphasis is on the explosive phases of supernovae. Part 1 is devoted to a survey of the kinds of observations that inform us about supernovae, some basic interpretations of such data, and an overview of the evolution of stars that brings them to an explosive endpoint. Part 2 goes into more detail on core-collapse and superluminous events: which kinds of stars produce them, and how do they do it? Part 3 is concerned with the stellar progenitors and explosion mechanisms of thermonuclear (Type Ia) supernovae. Part 4 is about consequences of supernovae and some applications to astrophysics and cosmology. References are provided in sufficient number to help the reader enter the literature.