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Be STARS
Proceedings of IAU Symposium No. 98 held in Munich, Federal Republic of Germany, April 6-10, 1981
Be and Shell Stars
The International Astronomical Union Symposium No. 70 on Be and Shell Stars, the Merrill-McLaughlin Memorial Symposium, was held in Bass River (Cap Cod), Massachusetts, U. S. A. , from September 15th through 18th, 1975. Fifty-three astronomers from Argentina, Belgium, Canada, Czechoslovakia, France, Israel, the United Kingdom, the United States, and the Vatican attended and participated in the Symposium. This volume, which parallels the actual program closely, contains the papers presented at the Symposium plus most of the discussion following the papers. New observational techniques and fresh theoretical ideas have resulted over the past few years in a renewed interest in Be and shell stars...
There Will Be Stars
“IN A LIFE FULL OF LIES, HE FINALLY SETTLED FOR THE TRUTH.” No one in Mattingly ever believed Bobby Barnes would live to see old age. Drink would either rot Bobby from the inside out or dull his senses just enough to send his truck off the mountain on one of his nightly rides. Although Bobby believes such an end possible—and even likely—it doesn’t stop him from taking his twin sons Matthew and Mark into the mountains one Saturday night. A sharp curve, blinding headlights, metal on metal, his sons’ screams. Bobby’s final thought as he sinks into blackness is a curious one—There will be stars. Yet it is not death that greets him beyond the veil. Instead, he returns to the day he has just lived and finds he is not alone in this strange new world. Six others are trapped with him. Bobby soon discovers that this supposed place of peace is actually a place of secrets and hidden dangers. Along with three others, he seeks to escape, even as the world around him begins to crumble. The escape will lead some to greater life, others to endless death . . . and Bobby Barnes to understand the deepest nature of love.
Spectral Atlas for Amateur Astronomers
A full colour reference featuring detailed commented spectral profiles of more than one hundred astronomical objects.
How the Stars Came to Be
New into paperback! HAVE YOU EVER WONDERED HOW THE STARS CAME TO BE? The Fisherman's Daughter loved to dance in the sunlight, and bathe in the glow of the moon, but when the moon disappeared for a few nights each month, she worried about her father and how he would find his way home from the sea in the darkness of the night. One night the sun finds her sobbing and so he takes one of his rays and smashes it onto the ground, creating the stars and gives the girl the task of putting them into the dark night sky. This beautifully illustrated story gives us a new folk tale, and a new way to look up at the night sky.
The Astrophysics of Emission-Line Stars
Emission line stars are attractive to many people because of their spectacular phenomena and their amazing varieties and variability. This book offers general information on emission line stars, starting from a brief introduction to stellar astrophysics and then moving to a broad overview of emission line stars including early and late type stars as well as pre-main sequence stars.
Evolution of Massive Stars
Massive stars occupy an exceptional place in general astrophysics. They trigger many if not all of the important processes in galactic evolution whereas due to their intrinsic brightness, they offer the (only until now) possibility to study the stellar content and stellar behaviour in distant galaxies. The last, say, 25 years, massive stars have been the subject of numerous meetings discussing the influence of massive stars on population synthesis, the number distribution of different types of massive stars, the LBV phenomenon, WR stars, X-ray binaries, stellar winds in massive stars, chemical pecularities in massive stars, supernova explosions of massive stars and the important SN1987A even...
The Classification of Stars
The classification of stars into their various types is one of the fundamental areas of astronomy. This book is a comprehensive handbook on the tools, methods and results of stellar taxonomy. Although this subject is firmly rooted in classical astronomy, vast improvements in observational techniques have transformed the subject and greatly broadened the wavelength regions available for study. The first six chapters describe modern methods of spectroscopic and photometric classification. The remaining nine chapters describe particular families of stars, progressing from the hottest to the coolest. Within each category a description is given of the normal type and all the peculiar stars. Throughout the emphasis is on the phenomenology of classification, rather than the underlying astrophysics. Both authors have devoted themselves to developing the international centre for stellar data at Strasbourg, which uniquely qualifies them to write this definitive handbook for professional astronomers.
Astronomy and Astrophysics Abstracts
Astronomy and Astrophysics Abstracts, which has appeared in semi-annual volumes since 1969, is devoted 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 documenta tion 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 ...
The Environments of the Sun and the Stars
Based on lectures given at a CNRS summer school in France, this book covers many aspects of stellar environments (both observational and theoretical) and offers a broad overview of the field. More specifically, Part I of the book focuses on the Sun, the properties of the ejected plasma, of the solar wind and on space weather. The second part deals with tides in planetary systems and in binary stellar systems, as well as with interactions in massive binary stars as seen by interferometry. Finally the chapters of Part III discuss the environments of young or evolved stars, stellar winds, agnetic fields and disks. With its broad approach the book will provide advanced students as well as researchers with a good overview of the environments of the Sun and the stars.
