Astronomy, space and time

This volume contains papers presented at IAU Colloquium No.

Continuum radio emission and fine structure (in particular millisecond spikes) have recently raised interest as diagnostic tools for the interpretation of energy release and particle acceleration in flares.

It was a general feeling among those who attended the NATO / ARW meeting on the Galaxy Distances and Deviations from Universal Expansion, that during the week in Hawaii a milestone had been passed in work on the distance scale.

If you want to understand the invisible, look careful at the visible.

"e;Fundamental Astronomy and Solar System Dynamics"e;, a program of invited papers honoring Professor Walter Fricke, who for thirty years has been Director of the Astronomisches Rechen lnstitut in Heidelberg, was held at the Thompson Conference Center of the University of Texas at Austin on Wednesday 27 March 1985 on the occasion of his seventieth birthday and retirement as Director of ARl.

'Light on Dark Matter', held from 10-14 June 1985 in the Dutch seaside resort of Noordwijk, was the first international conference devoted to the results of the all-sky survey by the US-Dutch-UK Infra-Red Astronomical Satellite (IRAS).

As it was said by one of the participants to this workshop"e; In our attempts to understand the spectral evolution of galaxies, we are fortunate indeed to have the ability to look back in time and observe galaxies as they were billions of years ago.

The idea to hold a conference on the Evolution of Close-Binary X-ray sources grew in the summer of 1984.

Plant hormone research is the favorite topic of physiologists.

This is a textbook on classical mechanics at the intermediate level, but its main purpose is to serve as an introduction to a new mathematical language for physics called geometric algebra.

This book sets forth and builds upon the fundamentals of the dynamics of natural systems in formulating the problem presented by Jacobi in his famous lecture series "e;Vorlesungen tiber Dynamik"e; (Jacobi, 1884).

The near Infra-Red emission of the Interstellar Medium is a very puzzling subject.

The idea for organl.

The first helium star was discovered in 1942, the first scientific meeting on the subject, however, took place in 1985.

The XIXth General Assembly of the International Astronomical Union was held in New Delhi, India, from November 19 to 28, 1985.

Algol is a triple system containing a 70 hr eclipsing binary (K IV and B8 V) in a 694 day orbit with an A V star.

Since 1976 a meeting devoted to recent research on cataclysmic variables ("e;CV workshop"e;) has been held annually somewhere in North America.

The 19th ESLAB Symposium on 'The Sun and the Heliosphere in Three Dimensions' was held in Les Diablerets (Switzerland) on 4-6 June 1985.

The history of modern helioseismology is only ten years old.

This volume is the documentation of the first Course on 'Neutron Stars, Active Galactic Nuclei and Jets', of an Erice School with a wide astro- physical scope.

The Milky Way Galaxy offers a unique opportunity to study the structure and contents of a major stellar system in three dimensions, at high spatial and spectral resolution, and to very large galactocentric distances.

This volume is based on the proceedings of the "e;NATO- Advanced study Institute on Mineral Processing Design"e; held in Bursa-Turkey on August 24-31, 1984.

Helio- and asteroseismology study the interior of the Sun and other stars, by means of observations of oscillations on their surfaces.

IAU Symposium 127 was held in Princeton on May 28-31, 1986, at the Institute for Advanced Study.

This book is the result of a meeting held in August, 1986 in Irsee, West Germany.

On April 28 1986 Cornelis de Jager reached the age of 65 years.

There are two questions that we can ask ourselves in order to describe this workshop.

The Symposium was held at the Great Wall Sheraton Hotel in Beijing, China in the period August 25-30, 1986.

An Advanced Research Workshop on Very High Energy Gamma Ray Astronomy and Related Topics was held at Durham, England during August 11-15 1986.

Over the last decade we have witnessed a rapid change in our understanding of the late stages of stellar evolution.

Recent advances in observational and theoretical efforts in understanding the nature of cataclysmic variables had reached such maturity that there existed a strong, shared feeling among the workers in this field that an international colloquium sponsored by the International Astronomical Union would be timely.

Interest in statistical methodology is increasing so rapidly in the astronomical community that accessible introductory material in this area is long overdue.

TH.

This book was conceived to commemorate the continuing success of the guest observer program for the International Ultraviolet Explorer (IUE) satellite observatory.

The same kind of physics is frequently common to very different fields of Astrophysics, so experts in each of these fields have often much to learn from each others.

This volume contains all but one of the lectures and seminars presented at the NATO Advanced Study Institute on HOI Thin Plasmas in Astrophysics held in Cargese, Corsica, from September 8 to 18, 1987.

This book represents the Proceedings of the NATO Advanced Study Insti- tute on Formation and Evolution of Low Mass Stars held from 21 September to 2 October 1987 at Viana do Castelo, Portugal.

This volume consists of invited talks and contributed papers presented at the NATO Advanced Study Institute "e;The Post Recombination Universe"e; which was held in Cambridge in the summer of 1987.

Astrophysical analysis relating to solid matter requires data on properties and processes.

Stellar mass loss is an essential part of the cycling of material from the interstellar medium into stars and back, and must be understood if we are to model processes on galactic to cosmological scales.

The millimetre and submillimetre spectral region (300 to 3000 Ilm or 1000 to 100 GHz) was until recently one of the few spectral regimes not fully opened up for astronomical studies.

Recent advances in the instrumentation used to observe star forming regions in both our own Milky Way and in external galaxies have transformed the subject from a phenomenological pursuit into an increasingly unified, physical science.