Starsdown


Book Description

Poetry. Jasper Bernes's magnificent and multi-layered first book, STARSDOWN, emerges as a record of Los Angeles as its physical space collapses into specters and marks, where "the sky is a swimming pool" and the signs and stars keep switching places. Beneath the glittering surface of the last American city, this book animates the profusion of irreconcilable vernaculars and histories that the city's "pastel-washed meta-burglaries" have contrived to make disappear. An archaeology of futures past and futures to come, STARSDOWN improvises a poetry which stands finally as actual invention and possibility.




The Stars Down Under


Book Description

Alien artifacts, political tension, and a freshly married pair of heroes populate this sequel to the military-adventure science fiction novel, "The Outback Stars."




The Stars Down to Earth


Book Description

The Stars Down to Earth shows us a stunningly prescient Adorno. Haunted by the ugly side of American culture industries he used the different angles provided by each of these three essays to showcase the dangers inherent in modern obsessions with consumption. He engages with some of his most enduring themes in this seminal collection, focusing on the irrational in mass culture - from astrology to new age cults, from anti-semitism to the power of neo-fascist propaganda. He points out that the modern state and market forces serve the interest of capital in its basic form. Stephan Crook's introduction grounds Adorno's arguments firmly in the present where extreme religious and political organizations are commonplace - so commonplace in fact that often we deem them unworthy of our attention. Half a century ago Theodore Adorno not only recognised the dangers, but proclaimed them loudly. We did not listen then. Maybe it is not too late to listen now.




The Stars Below (Vega Jane, Book 4)


Book Description

THIS. MEANS. WAR. The explosive conclusion to David Baldacci's instant #1 worldwide bestselling and award-winning fantasy series. From the beginning, the fight was coming. Vega Jane fought her way out of the village where she was born, crossed a wilderness filled with vicious creatures, and raised a ragtag army behind her. But each triumph earned through grit and pain only brought her closer to him.Necro. A sorcerer whose unspeakable evil is matched only by his magical power.Vega and Necro are on a collision course. The clash between his awesome power and her iron will is going to shake the stars down. Their fight will seal their fates . . . and determine the future of their world. The battle rages in The Stars Below, the furious conclusion to legendary storyteller David Baldacci's #1 global bestselling Vega Jane series.




The Story of the Stars


Book Description




Variable Stars in Globular Clusters and in Related Systems


Book Description

This volume contains the papers and discussions at IAU Colloquium No. 21 on Variable Stars in Globular Clusters and in Related Systems held in Toronto on the 29th, 30th and 31st August 1972. It was the intention of the organizers that this meeting should honour the life long work in this field of Professor Helen Sawyer Hogg. She has been continuously active in observational research on variables in globular clusters for 46 years and her catalogues and bibliographies as well as her research papers, review articles and IA U reports as chairman of the committee on variable stars in clusters are of fundamental importance to all workers in this field. The scope of the colloquium covered both observational and theoretical aspects of the problem, including the relationship of variables to non-variable cluster members, the position of the variables in the HR diagram and their importance for problems of stellar evolution, empirical data on the variables, periods and period changes, and the relevant parts of pulsation theory. The meeting was particularly successful in bringing together observers and theorists. It will have achieved its object if it has shown both observers and theorists which are the problems most suitable for attack at the present time. The meeting clearly demonstrated the great importance of research on variables in globular clusters and related systems for our understanding both of stellar evolution and stellar pulsation.




Observing Variable Stars, Novae and Supernovae


Book Description

Gerald North's complete practical guide and resource package instructs amateur astronomers in observing and monitoring variable stars and other objects of variable brightness. Descriptions of the objects are accompanied by explanations of the background astrophysics, providing readers with real insight into what they are observing at the telescope. The main instrumental requirements for observing and estimating the brightness of objects by visual means and by CCD photometry are detailed, and there is advice on the selection of equipment. The book contains a CD-ROM packed with resources, including hundreds of light-curves and over 600 printable finder charts. Containing extensive practical advice, this comprehensive guide is an invaluable resource for amateur astronomers of all levels, from novices to more advanced observers. Gerald North is a lifelong amateur astronomer. In addition to being a member of the British Astronomical Association since 1977, he is also the author of many books, including Advanced Amateur Astronomy (Cambridge, 1997) and Observing the Moon (Cambridge, 2000).




The Impact of Long-Term Monitoring on Variable Star Research


Book Description

Long-term monitoring is of fundamental significance in solving many important problems in astrophysics and, furthermore, has unequalled value in extending observational runs with small telescopes for the education of young astronomers in order to teach them how to secure high-quality observational data over many years. The Impact of Long-Term Monitoring on Variable Star Research contains reports based on the analysis of data collected in the visible, IR and radio measurement ranges, as well as the design and history of well known photometric systems. Though the reporting of novel results forms an important part of the book, there are also reports of eight discussion sessions covering more general areas, such as extinction monitoring, the problems of archival storage of astronomical data, service observation, the role played by long-term monitoring in graduate teaching and thesis supervision, the interplay between the great observational effort and theory, the contribution of LTM to new knowledge of fundamental data, and the increasing decommissioning of telescopes of modest aperture.




Petroglyphs and the Stars in Northumberland


Book Description

Cup and ring petroglyphs are found widely in Northumberland, Scotland, Ireland, Brittany, Spain, Portugal and further afield across the globe. They are mysterious and beautiful objects of art in the landscape, but, as this book explains, they are much more than that. Nine petroglyph sites in Northumberland are examined here, and are shown to have depicted the night sky above them in the Neolithic era to a high degree of accuracy. This opens up a whole new field of study because, together, the Northumberland petroglyphs make up a star atlas. Decoding them is likely to yield valuable astronomical information about the sky 4,500 years ago. This book provides the relevant astronomical background and explains carefully how these petroglyph motifs can be deciphered. It will be of interest to astronomers, archaeologists, conservationists of ancient monuments, and particularly to amateurs who would like a field guide on how to interpret the messages on these rocks for themselves.




Angular Momentum Evolution of Young Stars


Book Description

This book reports the Proceedings of the NATO Advanced Research Workshop on "An gular Momentum Evolution of Young Stars" held from 17 to 21 September 1990 at Noto, Italy. The workshop had its immediate origin in a discussion about the availability of stel lar rotation data, that took place in 1987 at Viana do Castelo Portugal during the NATO meeting, Formation and Evolution of Low Mass Stars. We recognized that nearly 20 years had passed since the last meeting on stellar rotation and that significant progress in the observation of rotation rates in low mass stars had been made. During the last 20 years, new efficient instrumentation (CCD and photon counting de tectors and echelle spectrographs) and new analysis techniques (profile Fourier analysis) have allowed us to measure rotational velocities as low as 1-2 km/s and to reach low mass stars in young clusters. Even with these advances, rotational velocities of low mass stars would have remained challenging to determine if all single, low mass stars later than GO had rotational velocities of order or less than 10 km/sec. Evidence that this is not always the case was first provided by the photometric variability data obtained by van Leeuwen and Alphenaar for K dwarfs in the Pleiades and more recently by the vsini measurements of low mass stars in several young clusters.