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This book presents an up-to-date detailed description and categorisation of the large range of astronomical objects that fall under the general heading of nebulae, and then instructs the reader in the best ways to successfully observe and record them. Nebulae and How to Observe Them is a comprehensive mine of information for all levels of amateur observers, from the beginner to the experienced.
Each note brings her one step closer to the truth. When the cyborg Nebula plays the piano she experiences memories from a time before her creation. These memories—which involve a captive rebel fighter being held on their ship—bring with them complex human feelings and awaken a desire for her to discover her origins. Radian is the long-lost love of the woman from which Nebula was made. He's vowed to avenge his finance's death and rescue her sister from the Gryphonites, a fierce race out to enslave the galaxy. Nebula grapples with her identity and how much of who she is comes from someone else's past. She is not the woman that died, yet she is undeniably drawn to Radian. Together Nebula and Radian seek to rescue his fiancé's sister and end the Gryphonites' cruel reign. But can Radian learn to love again and can Nebula accept a past made from someone else's memories? 30,453 Words
The Orion Nebula is the closest center of massive star formation—a stellar nursery that reproduces the conditions in which our own Sun formed some 4.5 billion years ago. In this book, O’Dell explains what the Nebula is, how it shines, its role in giving birth to stars, and the insights it affords into how common (or rare) planet formation might be.
Proceedings of IAU Symposium No. 76 held at Cornell University, Ithaca NY, USA, 6-10 June 1977
Thoroughly revised and expanded throughout, the new edition is a graduate-level text and reference book on gaseous nebulae, nova and supernova remnants. Much of the new data and new images are from the Hubble Space Telescope with two wholly new chapters being added along with other new features. The previous edition which was tried and tested for thirty years has now been succeeded by a revised, updated, larger edition, which will be valuable to anyone seriously interested in astrophysics.
In view of the current and forthcoming observational data on pulsar wind nebulae, this book offers an assessment of the theoretical state of the art of modelling them. The expert authors also review the observational status of the field and provide an outlook for future developments. During the last few years, significant progress on the study of pulsar wind nebulae (PWNe) has been attained both from a theoretical and an observational perspective, perhaps focusing on the closest, more energetic, and best studied nebula: the Crab, which appears in the cover. Now, the number of TeV detected PWNe is similar to the number of characterized nebulae observed at other frequencies over decades of observations. And in just a few years, the Cherenkov Telescope Array will increase this number to several hundreds, actually providing an essentially complete account of TeV emitting PWNe in the Galaxy. At the other end of the multi-frequency spectrum, the SKA and its pathfinder instruments, will reveal thousands of new pulsars, and map in exquisite detail the radiation surrounding them for several hundreds of nebulae. By carefully reviewing the state of the art in pulsar nebula research this book prepares scientists and PhD students for future work and progress in the field.