Black Holes, White Dwarfs, and Neutron Stars


Book Description

This self-contained textbook brings together many different branches of physics--e.g. nuclear physics, solid state physics, particle physics, hydrodynamics, relativity--to analyze compact objects. The latest astronomical data is assessed. Over 250 exercises.










Understanding Stellar Evolution


Book Description

'Understanding Stellar Evolution' is based on a series of graduate-level courses taught at the University of Washington since 2004, and is written for physics and astronomy students and for anyone with a physics background who is interested in stars. It describes the structure and evolution of stars, with emphasis on the basic physical principles and the interplay between the different processes inside stars such as nuclear reactions, energy transport, chemical mixing, pulsation, mass loss, and rotation. Based on these principles, the evolution of low- and high-mass stars is explained from their formation to their death. In addition to homework exercises for each chapter, the text contains a large number of questions that are meant to stimulate the understanding of the physical principles. An extensive set of accompanying lecture slides is available for teachers in both Keynote(R) and PowerPoint(R) formats.




Snow White and the 77 Dwarfs


Book Description

Snow White is on the run from an evil witch when she comes across some dwarfs in the forest. They agree to take her in and keep her safe if she will help them with their chores. She soon realizes she's taking on a lot more than she bargained for. 77 breakfasts to make, 77 lunches to pack (don't forget the juice boxes!), 77 pairs of pants to mend and a whole lot of dishes. Eventually Snow White decides to take her chances with the witch. There's a surprise ending... well, it may not be so surprising. This is a hilarious retelling of the classic tale, with bright, energetic illustrations featuring busy dwarfs, and the even busier Snow White.




White Dwarfs


Book Description

Proceedings of the NATO Advanced Research Workshop, held in Naples, Italy, 24-28 June 2002




From White Dwarfs to Black Holes


Book Description

From White Dwarfs to Black Holes chronicles the extraordinarily productive scientific career of Subrahmanyan Chandrasekhar, one of the twentieth century's most distinguished astrophysicists. Among Chandrasekhar's many discoveries were the critical mass that makes a star too massive to become a white dwarf and the mathematical theory of black holes. In 1983 he shared the Nobel Prize for Physics for these and other achievements. Over the course of more than six decades of active research Chandrasekhar investigated a dizzying array of subjects. G. Srinivasan notes in the preface to this book that "the range of Chandra's contributions is so vast that no one person in the physics or astronomy community can undertake the task of commenting on his achievements." Thus, in this collection, ten eminent scientists evaluate Chandrasekhar's contributions to their own fields of specialization. Donald E. Osterbrock closes the volume with a historical discussion of Chandrasekhar's interactions with graduate students during his more than quarter century at Yerkes Observatory. Contributors are James Binney, John L. Friedman, Norman R. Lebovitz, Donald E. Osterbrock, E. N. Parker, Roger Penrose, A. R. P. Rau, George B. Rybicki, E. E. Salpeter, Bernard F. Schutz, and G. Srinivasan.




Mass Loss and Evolution of O-Type Stars


Book Description

The organization of this Symposium had its beginnings at the International Astronomical Union General Assembly in Grenoble in 1976. The initial "rounding up" of the Scienti fic Organizing Committee was begun by Drs. Snow and Swings; most of us who became the eventual organizing committee met a few times during the Assembly and formulated the essential outlines of the meeting. Extensive correspondence with all the committee subsequently established the program. The idea was to bring together both observers and theoreticians to discuss the stellar winds and mass loss rates and their effects on evolutions of O-type stars. On the observational side, there are now spectroscopic data from the far UV to the near IR regions concerning the stellar winds. There is also information about the free-free emission in the wind from the IR and radio portions of the spectrum. Fortunately, these different detection methods give more or less the same mass loss rate for the one star, s Pup" which has been observed at all wavelengths. One of the intents of the first three sessions of this Symposium is to outline the eXisting data on mass loss rates as it per tains to the O-type stars.




Literature 1980, Part 1


Book Description

Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is de voted to the recording, summarizing and indexing of astronomical publications throughout the world. It is prepared under the auspices of the International Astronomical Union (according to a resolution adopted at the 14th General Assembly in 1970). Astronomy and Astrophysics Abstracts aims to present a comprehensive documentation of literature in all fields of astronomy and astrophysics. Every effort will be made to ensure that the average time interval between the date of receipt of the original literature and publication of the abstracts will not exceed eight months: This time interval is near to that achieved by monthly abstracting journals, com pared to which our system of accumulating abstracts for about six months offers the advantage of greater convenience for the user. I, 1980; some older Volume 27 contains literature published in 1980 and received before August literature which was received late and which is not recorded in earlier volumes is also included. We acknowledge with thanks contributions to this volume by Dr. J. Bouska, Prague, who surveyed journals and publications in Czech and supplied us with abstracts in English.




The Fairest One of All


Book Description

In 2012 Disney celebrated the 75th anniversary of the Snow White movie, a beloved classic and an important milestone in film history. This book, created with the Walt Disney Family Foundation, run by Walt’s daughter, is an exploration of the making of the film that includes never-before-published facts and art. The Fairest One of All won the award for Best Animation Book at the 2012 A113Animation Awards. Walt Disney’s Snow White and the Seven Dwarfs was first shown to a theatrical audience in December 1937 and brought overwhelming, joyous applause from a house full of hardened film-industry professionals. In subsequent months it would open around the world, happily acclaimed by audiences and critics everywhere as one of the best films of the year, if not the decade. From today’s perspective, its stature is even greater—named as one of the best movies of all time by the American Film Institute, and still beloved by children and adults around the world, Snow White can be seen as the flowering of an all-too-brief Golden Age of animation as well as a fascinating document of its time. Such a level of artistic achievement doesn’t happen by accident. Walt Disney and a staff of exceptionally talented artists labored over Snow White for four years, endlessly working and reworking their scenes to achieve an ever higher standard. The result, as we know, was magnificent and game-changing for the Disney Studios and, indeed, for the art of animation itself. This book is the first to reconstruct that process in exacting detail, with the loving attention it deserves from an internationally noted film scholar. Author J.B. Kaufman spent years researching the film’s history, interviewing participants, and studying the marvelous archival art that appears in these pages. The result is a work that can be appreciated equally as a piece of film history and as a collectable art book, a joy for anyone who loves film, animation, and the magical world that Walt Disney created.