The Galaxy

'One of the greatest achievements in comedy. A work of staggering genius' - David Walliams An international phenomenon and pop-culture classic, The Hitchhiker's Guide to the Galaxy has been a radio show, TV series, novel, stage play, comic book and film. Following the galactic (mis)adventures of Arthur Dent, Hitchhiker’s in its various incarnations has captured the imaginations of curious minds around the world . . . It's an ordinary Thursday lunchtime for Arthur Dent until his house gets demolished. The Earth follows shortly afterwards to make way for a new hyperspace express route, and his best friend has just announced that he's an alien. At this moment, they're hurtling through space with nothing but their towels and an innocuous-looking book inscribed, in large friendly letters, with the words: DON'T PANIC. The weekend has only just begun . . . This 42nd Anniversary Edition includes exclusive bonus material from the Douglas Adams archives, and an introduction by former Doctor Who showrunner, Russell T Davies. Continue Arthur Dent's intergalactic adventures in the rest of the trilogy with five parts: The Restaurant at the End of the Universe, Life, the Universe and Everything, So Long, and Thanks for All the Fish, and Mostly Harmless.

In this exquisite volume, the intricate and beautiful fashions that have appeared in all six "Star Wars(" films are on display--from military gear to royal gowns and the iconic garbs of Obi-Wan Kenobi and Darth Vader.

In this gripping and spectacular rollercoaster of an adventure, a fourteen-year-old Earth boy is chosen, seemingly at random, to become Emperor of the Galaxy during a time of grave peril. Spencer, an ordinary teenager, lives with his mum, his stepdad Hassan and his younger brother Mo. He is decidedly average at school, sports and at video gaming, but when he is chosen to become the new Emperor of the Galaxy everything changes. Spencer must learn how to balance being Emperor of the Galaxy and battle the evil Haxenaar, trying to get his homework in on time, and all the while pursuing the love of his life, Amy Heartly. With the help of his new companions and Bradlii, the smartest and smuggest AI ever created, Spencer must brave an epic journey to save the galaxy and discover the ultimate truth.

In published papers H A Bethe and G E Brown worked out the collapse of large stars and supernova explosions. They went on to evolve binaries of compact stars, finding that in the standard scenario the first formed neutron star always went into a black hole in common envelope evolution. C-H Lee joined them in the study of black hole binaries and gamma ray bursts. They found the black holes to be the fossils of the gamma ray bursts. From their properties they could reconstruct features of the burst and of the accompanying hypernova explosions.This invaluable book contains 23 papers on astrophysics, chiefly on compact objects, written over 23 years. The papers are accompanied by illuminating commentary. In addition there is an appendix on kaon condensation which the editors believe to be relevant to the equation of state in neutron stars, and to explain why black holes are formed at relatively low masses.

The Galaxy Defenders is a group that helps the Galactic Government protect the known universe. However, the members of the Defenders have their hands full when a few powerful Empires come to power From the destruction of the gigantic Planet Blasters to the the final battle at Capital Planet, this book tells of the early struggles of the Galaxy Defenders to defend the Galactic Government and the known universe.

The morphological scheme devised by Hubble and followers to classify galaxies has proven over many decades to be quite effective in directing our quest for the fundamental pa rameters describing the extragalactic manifold. This statement is however far more true for spirals than for ellipticals. Echoing the concluding remarks in Scott Tremaine's sum mary talk at the Princeton meeting on Structure and Dynamics of Elliptical Galaxies, "the Hubble classification of spirals is useful because many properties of spirals (gas con tent, spiral arm morphology, bulge prominence, etc. ) all correlate with Hubble time. By contrast, almost nothing correlates with the elliptical Hubble sequence El to E7. " During the last few years much effort has been put into the search for a more meaningful classification of ellipticals than Hubble's. Concomitantly, forwarded by some provocative conjectures by R. Michard, the classical question of whether E galaxies form a physically homogeneous family has been brushed up once more. Results of these and other parallel studies look rather promising and point to suture part of the dichotomy between ellipticals and disk galaxies which had become popular in the early eighties, owing to dynamical arguments. At the same time it appears more and more clear that, besides the usual genetic varieties of galaxies, products of environmental evolution must also be contemplated in building our modern picture of the "reign of galaxies" . The above considerations prompted us to solicit Prof.