It is March 1998 and Chic Lucas is down on his luck. He has endured three major losses within a short period of time: the death of his father, a divorce, and the loss of his long-time job. Heartsick at his recent defeats, Chic is embarking on a quest to replenish his soul by returning to Poland, the land of his parents tribulations, to learn more about his familys life during World War II. As his journey takes him from Kansas City to Poland, Chics path crosses with that of a Jewish-American woman, Ruth Mintz, who is there to commemorate her mothers experiences as a Holocaust survivor. As Chics eyes are opened to the anti-Semitism of some Polish people and the animosity many Jewish people hold toward the Poles, he and Ruth become romantically involved. While each sets down different yet equally enlightening trails to the truth, their relationship becomes complicated by the disparities in their backgrounds, leaving Chic and Ruth to decide whether they can overcome their challenges and move forward into the future together. In this compassionate tale of courage and survival, the paths of two strangers intertwine in Poland where each is searching for insight into a horrible period in history.

Originally published in 1946, this book explains important aspects of the world through the lens of mathematics. McKay discusses important questions such as time, the size of the earth and 'numbers that mean too much' in language that is enthusiastic and easily accessible to non-mathematicians. This book will be of value to anyone with an interest in the history of mathematics.

Fifty thousand years ago, a small family of our ancestors huddled around a campfire. Robbed of vision, they were vulnerable in the darkness; the night is the time of the predator. As they listened to the crackle of the fire and the sounds of the night, they looked upwards. What, they wondered, were those mysterious lights in the sky? So begins astronomer Richard Hall's engrossing account of the stars as seen from Down Under! Today scientists know a great deal about the universe we live in. Photos have even been taken of the planet Mars, 35 million miles away. But for most people it's all still a mystery.

Classical stellar evolution theories have undergone some drastic changes in recent decades. New insights into the development of stellar interiors were obtained from studying stars in various stages of their lives, as well as with the help of fast computers, which gave a boost to the branch of numerical modelling of stellular structure and evolution. This book is divided into two parts. The first part deals with the general aspects of stellular structure and evolution including a chapter on numerical modelling. The second part deals with specific evolutionary aspects of single and binary stars with a variety of masses. The last chapter gives several models of stars with specific masses. The book is intended as an introduction for students, as well as a reference for researchers.

Stars are the fundamental observable constituents of the Universe. They are the first objects we see in the night sky, they dominate the light produced in our own and other galaxies, and nucleosynthesis in stars produces all the elements heavier than helium. A knowledge of stars and their evolution is vital to understand other astrophysical objects from accreting black holes and galaxies to the Universe itself.The structure of a star can be described mathematically by differential equations derived from the principles of hydrodynamics, electromagnetic theory, thermodynamics, quantum mechanics, atomic and nuclear physics. The basic equations of a spherical star are derived in detail at an accessible level. The topics discussed include modes of energy transport, the equation of state, the physics of the opacity sources and the nuclear reactions. Attention is also given to the virial theorem, polytropic gas spheres and homology principles and the procedure for numerical solution of the equations is outlined. This book tracks the evolution of stars from their main-sequence evolution through the exhaustion of various nuclear fuels to the end points of evolution and also introduces the topic of interacting binary stars. The aim is to take the reader from the essential underlying physical principles to the doors to current research on stellar interiors.

When the Executive Committee of the International Astronomical Union asked me, in 1968, to organize a Symposium on White Dwarfs it became evident that members of at least four Commissions of the IAU should participate, and that the most oppor tune place, and time to hold such a Symposium would be somewhere in the British Isles and just preceding the Fourteenth General Assembly at Brighton in August, 1970. After a preliminary correspondence with Dr. D. W. N. Stibbs it was decided to accept his invitation to hold the Symposium at St. Andrews University, Scotland, while the dates 11-13 August 1970 were selected. I am sure I speak for all the partici pants of the Symposium when I express our deep gratitude to Dr. Stibbs for the admirable way in which he planned and organized this meeting down to the smallest details - the success of the conference is due in no small measure to his continuous and painstaking efforts. An organizing committee was formed, consisting of O. J. Eggen (Photometry), J. L. Greenstein (Spectroscopy), A. G. Masevitch (Stellar Interiors), V. Weidemann (Stellar Atmospheres), D. W. N. Stibbs (local chairman), with myself (Proper Motions and Parallaxes) as overall chairman.

This up-to-date volume offers student researchers an unexcelled primer on current scientific knowledge about stars. This volume in the Greenwood Guides to the Universe series provides the most up-to-date understanding available of the current knowledge about stars. Scientifically sound, but written with the student in mind, Stars is an excellent first step for young people researching the exciting scientific discoveries that continue to extend our knowledge of the universe. Stars is organized thematically to help students better understand these most interesting heavenly bodies. Stars discusses all areas of what is known about the subject. It will help student understand things such as white dwarfs, neutron stars, pulsars, and black holes. And it will answer student questions such as: Why do stars have different colors and how are they classified? How do we know what stars are made of? How did scientists figure out how stars evolved?