Evolutionary Processes in Binary and Multiple Stars

Erscheinungsjahr 2016
ISBN: 978-0-521-85557-0
Verlag: Cambridge University Press

Buch, Englisch, Band 40, 330 Seiten, Format (B × H): 175 mm x 250 mm, Gewicht: 754 g

Reihe: Cambridge Astrophysics

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 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.

Autoren/Hrsg.

Eggleton, Peter

Fachgebiete

• Naturwissenschaften Physik Angewandte Physik Astrophysik
• Naturwissenschaften Astronomie Galaxien und Sterne
• Naturwissenschaften Astronomie Astrophysik

Inhaltsverzeichnis

1. Introduction
2. Evolution of single stars
3. Binary interaction: conservative processes
4. Slow non-conservative processes
5. Rapid non-conservative processes
6. Accretion by the companion
Appendices.

Über Autor(innen)

Eggleton, Peter
Peter Eggleton is a physicist at the Lawrence Livermore National Laboratory in California.