Eggleton peter (20 Ergebnisse)

Paperback. Zustand: New.

Zustand: New.

Zustand: New.

Zustand: As New. Unread book in perfect condition.

Taschenbuch. Zustand: Neu. Neuware - In Peter Eggleton's hilariously wild To Hell and Back, Hell is a former Government department, once managed by the FBI but privatised under the Reagan administration. Satan is the CEO, but his organisation has inherited an unchangeable culture of paperwork, which often encroaches on the time his demons have for torturing damned souls. Thus nowadays he tries to prevent people selling their souls for power and money, but the demand is enormous: the product flies off the shelf.One group of sinners being boiled in oil in Hell, for all eternity, is dirty old men. After being boiled for a few weeks, they are sent to the Recovery Room for a skin graft, so that they can be boiled again; this treatment is called 'Satancare'. One possible candidate, not yet dead, is the jewelry magnate Wilbur Smith.…

Zustand: New.

Paperback. Zustand: New.

Zustand: New.

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, Illustrations. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 246 x 170 x 18. Weight in Grams: 548. . 2011. Paperback. . . . .…

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, Illustrations. BIC Classification: PGM; PHVB. Category: (P) Professional & Vocational. Dimension: 246 x 170 x 18. Weight in Grams: 548. . 2011. Paperback. . . . . Books ship from the US and Ireland.…

Taschenbuch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.…

Zustand: New.

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, 52 b/w illus. 28 tables. BIC Classification: PGM. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 19. Weight in Grams: 828. . 2006. Illustrated. hardcover. . . . . …

Zustand: New.

Zustand: As New. Unread book in perfect condition.

Hardback. Zustand: New. Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.…

Zustand: New. This 2006 volume discusses the statistics of binary stars; the evolution of single stars; and interaction between multiple stars. Series: Cambridge Astrophysics. Num Pages: 332 pages, 52 b/w illus. 28 tables. BIC Classification: PGM. Category: (P) Professional & Vocational. Dimension: 247 x 174 x 19. Weight in Grams: 828. . 2006. Illustrated. hardcover. . . . . Books ship from the US and Ireland. …

Hardcover. Zustand: Brand New. 1st edition. 330 pages. 9.75x7.00x0.75 inches. In Stock.

Buch. Zustand: Neu. Druck auf Anfrage Neuware - Printed after ordering - Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.…

Hardback. Zustand: New. Binary systems of stars are as common as single stars. Stars evolve primarily by nuclear reactions in their interiors, but a star with a binary companion can also have its evolution influenced by the companion. Multiple star systems can exist stably for millions of years, but can ultimately become unstable as one star grows in radius until it engulfs another. This volume, first published in 2006, discusses the statistics of binary stars; the evolution of single stars; and several of the most important kinds of interaction between two (and even three or more) stars. Some of the interactions discussed are Roche-lobe overflow, tidal friction, gravitational radiation, magnetic activity driven by rapid rotation, stellar winds, magnetic braking and the influence of a distant third body on a close binary orbit. A series of mathematical appendices gives a concise but full account of the mathematics of these processes.…