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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."

Since Harvey Cushing's extensive study on brain meningiomas no similar study has been conducted on spinal cord meningiomas. The high scientific value of this book is based on the careful elaboration of data from patients affected by spinal meningiomas who have been examined and operated on over the last 33 years (1962-1995) at the Neurosurgical School of the University of Florence, Italy. The main focus of this study was on the anatomic and clinical relationship that enabled early diagnosis of spinal meningiomas. More over this book emphasizes the interaction between neurology and neuroradiology in the form of "dynamic neurology." Myeloradiculographic findings are described together with those using more recent techniques such as CT and MRI.