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One approach to learning about stellar populations is to study them at three different levels of resolution. First in our own Galaxy; secondly from ne...Savoir plus
The study of the evolution of galaxies has made remarkable progress in recent years and is currently undergoing a transformation arising from the appl...Savoir plus
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The investigation of the Galactic nucleus and its surroundings is necessarily a modem endeavor, for traditional observations made at visual wavelength...Savoir plus
IAU Symposium No. 134 on Active Galactic Nuclei was hosted by the Lick Observatory, as part of the celebration of its centennial, for the Observatory ...Savoir plus
A few years ago, a motivation for organizing one more IAU Symposium on star for- mation in Grenoble, was the anticipated completion of the IRAM interf...Savoir plus
The 186th IAU Symposium came at an exciting and perhaps even historic time for extragalactic astronomy. New spacecraft observations plumbed the depths...Savoir plus
The atmospheres of many stars have chemical compositions that are significantly different from that of the interstellar medium from which they are for...Savoir plus
This symposium was devoted to a new celestial mechanics whose aim has become the study of such `objects' as the planetary system, planetary rings, the...Savoir plus
Highly ionized atoms in the general interstellar gas of the galactic disk were first detected through interstellar absorption line observations of 0 V...Savoir plus
The investigation of the Galactic nucleus and its surroundings is necessarily a modem endeavor, for traditional observations made at visual wavelength...Savoir plus
In the early summer of '89 a very informal meeting on the bulge of our Galaxy was held in Leiden. During that meeting Michael Rich proposed to hold a ...Savoir plus
Preface and Highlights. Historical Remarks. Resolutions Adopted. Space Optical Astrometry. Ground-Based Optical Astrometry. Very Long Baseline Interfe...Savoir plus
Foreword. Introductory Review. I: The Observational PN Database. II: Highlights on the Nuclei. III: Highlights on the Nebulae. IV: Planetary Nebulae C...Savoir plus
G. MICHAUD Dipartement de Physique Universiti de Montrial c. P. 6128, succursale A Montrial, Que., H3C 317 Canada The aim of IAU Symposium 145 was to ...Savoir plus
These proceedings offer professional astronomers an overview of the rapidly advancing subject of galaxy interactions at low and high redshifts. The sy...Savoir plus
Preface. 1. The Solar Dynamo. 2. Long-Term Variability of the Solar Magnetic Cycle. 3. Numerical Simulations of Convection and Dynamo Processes. 4. La...Savoir plus
The first ideas for the symposium were generated in Brussels in the summer of 1986, dur- ing exquisite lunches in between HST proposal consortium meet...Savoir plus
Active Galactic Nuclei radiate over the electro-magnetic spectrum from radio waves to gamma rays. Understanding the physics of these objects therefore...Savoir plus
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Stellar flares represent one of the most challenging problems of contemporary astrophysics. Both solar and stellar observations have shown the flare p...Savoir plus
G. MICHAUD Dipartement de Physique Universiti de Montrial c. P. 6128, succursale A Montrial, Que., H3C 317 Canada The aim of IAU Symposium 145 was to ...Savoir plus
The first ideas for the symposium were generated in Brussels in the summer of 1986, dur- ing exquisite lunches in between HST proposal consortium meet...Savoir plus