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Astronomy from Space
Since the Space Age began a quarter-century ago, astronomers have been able to reach out and often touch celestial bodies that formerly could only be dimly viewed from afar. Probes have flown by or landed on many of the planets. Astronauts have made direct observations from Earth orbit and on the Moon. Most important, a host of satellites in Earth orbit have recorded the emissions of X-ray, infrared, and ultraviolet radiation from distant sources normally invisible beneath the atmosphere. And when the Space Telescope goes aloft, man's vision of the cosmos will be extended further still. The essays in this book describe the results of twenty-five years of space observation, summarize what has...
High Resolution Infrared Spectroscopy in Astronomy
Two specialized new instruments for ESO's VLT, VISIR and CRIRES, spawned the idea for this workshop. CRIRES is a dedicated very high resolution infrared spectrograph; VISIR features a high resolution spectroscopic mode. Together, the instruments combine the sensitivity of an 8m-telescope with the now well-established reliability of VLT-facility instruments. High resolution here means that lines in cool stellar atmospheres and HII-regions can be resolved. The astrophysical topics discussed in this rather specialized workshop range from the inner solar system to active galactic nuclei. There are many possibilities for new discoveries with these instruments, but the unique capability, which bec...
Cyclical Variability in Stellar Winds
It is well known that stellar winds are variable, and the fluctuations are often cyclical in nature. This property seems to be shared by the winds of cool and hot stars, even though their outflows are driven by fundamentally different physical mechanisms. Since very similar models have been proposed to explain the cyclical wind variations observed in a wide variety of stars, the time was ripe for astrophysicists from many different sub-disciplines to present the state of the art in a concise form. The proceedings will provide a useful, up-to-date overview of the observations, interpretation, and modelling of the time-dependent mass outflows from all sorts of stars.
