D. A. Williams – författare

Molecules in the early Universe acted as natural temperature regulators, keeping the primordial gas cool and, in turn, allowing galaxies and stars to be born. Even now, such similarly simple chemistry continues to control a wide variety of the exotic objects that populate our cosmos. What are the tools of the trade for the cosmic chemist? What can they teach us about the Universe we live in? These are the questions answered in this engaging and informative guide, The Chemically Controlled Cosmos. In clear, non-technical terms, and without formal mathematics, we learn how to study and understand the behaviour of molecules in a host of astronomical situations. We study the secretive formation of stars deep within interstellar clouds, the origin of our own Solar System, the cataclysmic deaths of many massive stars that explode as supernovae, and the hearts of active galactic nuclei, the most powerful objects in the Universe. We are given an accessible introduction to a wealth of astrophysics, and an understanding of how cosmic chemistry facilitates the investigation of many of the most exciting questions concerning astronomy today.

Molecules in the early Universe acted as natural temperature regulators, keeping the primordial gas cool and, in turn, allowing galaxies and stars to be born. Even now, such similarly simple chemistry continues to control a wide variety of the exotic objects that populate our cosmos. What are the tools of the trade for the cosmic chemist? What can they teach us about the Universe we live in? These are the questions answered in this engaging and informative guide, The Chemically Controlled Cosmos. In clear, non-technical terms, and without formal mathematics, we learn how to study and understand the behaviour of molecules in a host of astronomical situations. We study the secretive formation of stars deep within interstellar clouds, the origin of our own Solar System, the cataclysmic deaths of many massive stars that explode as supernovae, and the hearts of active galactic nuclei, the most powerful objects in the Universe. We are given an accessible introduction to a wealth of astrophysics, and an understanding of how cosmic chemistry facilitates the investigation of many of the most exciting questions concerning astronomy today.

Liquid Fuels discusses the properties, classification, manufacturing, and practical use of liquid fuels. The book is organized into 10 chapters discussing the various aspects of liquid fuels, from source to storage. Chapters 1 and 2 present the main source of liquid fuels and other sources such as oil shales and coal. Chapter 3 illustrates the physical and chemical tests used to determine the properties of liquid fuels and the significance of these properties to the practical applications of the different types of fuels. Fuels for spark and compression ignition engines are discussed in Chapters 4 and 5. Chapter 6 presents the combustion and atomization of fuel oils. Chapters 7 to 9 enumerate the industrial and household uses of liquid fuels. The final chapter deals with the handling and storage of liquid fuels. Students of chemical engineering and metallurgy and people working at industries requiring the use of liquid fuels in their manufacturing processes will find the book useful.