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This comprehensive and unique reference work on astro-tomography is based on expanded and suitably edited contributions to the 1st International Workshop on Astro-tomography. The focus is on studying indirect imaging and subsequent reconstruction techniques with applications in all areas of observational astronomy, astrophysics and cosmology. Detailed subject and object indexes, together with a list of useful resources on the Internet, will help the reader to use this book in a most efficient way.
In 1993 we began to consider the possibility of holding a conference on Catacysmic Variables (CVs) at Keele University. There have been several meetings in the area of CVs recently (e. g. Eilat, Abano-Padova, Capetown). However as preparations for the Keele meeting progressed we realized that, while there had been a number of IAU meetings devoted to related and to peripheral topics (such as IAU Colloquium 122 on Classical Novae in 1989, IAU Colloquium 129 on Accretion Disks in 1990), there had been no IAU-sponsored conferences in the area of cataclysmi/: variables (CVs) for a number of years. We felt therefore that the time was ripe to have an IAU meeting de voted to an overview of CVs and r...
Titanium is a strong, lustrous, silvery-white metal that can be alloyed with other elements, such as iron and aluminum, to create strong but lightweight alloys for use in the aerospace, automotive, agricultural, medical, and sporting goods industries. Its most important properties are its resistance to corrosion and extremely high strength-to-weight ration, the highest of any metal. This book provides all the important bedrock information about titaniums properties, while also telling the story of its discovery and describing the wide variety of uses to which it is put, from jet engines and spacecraft to desalination plants, paper mills, prosthetic limbs, tennis rackets, and golf clubs.
What is it like to spend a lifetime doing research in a wide variety of fields in the physical sciences? Studying distant planets, binary stars, neutron stars, stellar mass black holes and active galaxies using optical and near-infrared ground-based telescopes. Designing and constructing equipment as a member of international teams studying the high-energy X-ray emissions from many of these objects. Flying these detectors on short duration sounding rocket flights, utilising huge balloons to carry experiments to high altitude, or installing them on long duration satellite missions. Being a scientist engaged in fieldwork studying the physical properties of the world’s oceans, or the sea ice and glaciers around the coastline of Antarctica. This lifetime involved living in the UK and Australia for many years, with a four-year interlude in the USA, as well as working in or visiting many other countries. How lucky can you get? This book describes numerous projects in an unusually diverse range of research areas – the fun and adventure of STEM activities – without getting into excessive technical or specialist detail.
Seated in a sun-lit corner of his 17th century Dutch house, his hand touching a celestial globe, Johannes Vermeer's "Astronomer" seems to pon der about the mysteries of the universe. We might make the trip to Paris and ask him, in the Louvre, what precisely is on his mind. Unfortunately, there will be no answer. But we do know what his mind was not on. It was not on the approaching deadlines for the proposals he would have to write for getting funds and telescope-time, not on the meeting of the observing programs committee, not on his refereeing duty for the journal Astronomy & Astrophysics, nor on his university's tightening budget for science. In the Kapteyn Institute at Groningen I stand face to face with the im pressive portrait of J.C. Kapteyn, painted in the year 1918. Seated at his desk he is doing his calculations with pen, pencil and tables, perhaps check ing the work of his skilled staff of human computers. Early in his career he had completed his magnum opus, the Cape Photographic Durchmusterung in collaboration with his close friend David Gill at Capetown, South Africa.
DIVDIVOn Mars, a research team encounters an ancient puzzle that only a guitarist can solve/divDIV/divDIV In 2029, an American research team ventures to Mars to investigate an astounding find: a labyrinth older than humanity itself, whose maze of rooms conceals the deepest secrets of the red planet. In the final chamber, strange music plays, as chilling as it is beautiful. It will be the last thing the scientist who discovers it ever hears. As the music rises to a climax, the chamber door closes, leaving him to die in the pitch dark./div Where one explorer has failed, Ben Cassidy must not. An internationally famous guitarist, his music is the closest thing on Earth to Mars’s deadly hymn. The government sends him into space to solve a planetary mystery, but what Cassidy encounters is a team of researchers whose jealous competition is every bit as dangerous as the secrets of Mars. /div
This book is a well-edited and comprehensive survey of the current research in the field of low-mass accretion powered compact binaries, that is, binary stars containing a white dwarf, neutron star, or black hole as the primary star and a Roche-lobe filling low-mass as the secondary star. These stars have reached a stage in their evolution where the transfer of mass from the giant phase onto a dwarf or sub-dwarf star demonstrates many different aspects of physics. The volume is essentially a complete analysis of these stars combining theory and observation, and covering observations of low-mass X-ray binaries and both magnetic and nonmagnetic cataclysmic variables, theories of stellar accretion, novae, and evolution of compact binaries.
From the beginning of Space Astronomy, the Extreme Ultraviolet band of the spectrum (roughly defined as the decade in energy from 90-900 Å) was deemed to be the `unobservable ultraviolet'. Pioneering results from an EUV telescope on the Apollo-Soyuz Mission in 1975 forcibly demonstrated that this view was incorrect; but it required the all-sky surveys of the English Wide-Field Camera and the Extreme Ultraviolet Explorer to demonstrate the broad potential of this field. Over 700 EUV sources have now been detected. Over 150 researchers from 16 countries gathered to share results in this new field at the International Astronomical Union Colloquium No. 152. Papers were presented on a wide variety of topics including cool star coronae, white dwarf atmospheres and evolution, neutron stars, the Io torus, cataclysmic variable stars, active galactic nuclei, the interstellar medium, winds and atmospheres of early type stars, and EUV plasma diagnostics. Selected manuscripts from this meeting are provided in these Conference Proceedings.
The proceedings of MG16 give a broad view of all aspects of gravitational physics and astrophysics, from mathematical issues to recent observations and experiments. The scientific program of the meeting included 46 plenary presentations, 3 public lectures, 5 round tables and 81 parallel sessions arranged during the intense six-day online meeting. All talks were recorded and are available on the ICRANet YouTube channel at the following link: www.icranet.org/video_mg16.These proceedings are a representative sample of the very many contributions made at the meeting. They contain 383 papers, among which 14 come from the plenary sessions.The material represented in these proceedings cover the fol...