Skip to main content
Book cover

An Introduction to the Evolution of Single and Binary Stars

  • Textbook
  • © 2013

Overview

  • Introduces the physics behind single and binary stellar evolution, assuming no prior knowledge of astronomy
  • Focuses on the evolution of stars to the end point of white dwarf, neutron star, and black hole binary systems
  • Fills the niche between more-and-less advanced books, currently available on the topic
  • Includes supplementary material: sn.pub/extras

Part of the book series: Undergraduate Lecture Notes in Physics (ULNP)

This is a preview of subscription content, log in via an institution to check access.

Access this book

eBook USD 44.99
Price excludes VAT (USA)
  • Available as PDF
  • Read on any device
  • Instant download
  • Own it forever
Softcover Book USD 59.99
Price excludes VAT (USA)
  • Compact, lightweight edition
  • Dispatched in 3 to 5 business days
  • Free shipping worldwide - see info

Tax calculation will be finalised at checkout

Other ways to access

Licence this eBook for your library

Institutional subscriptions

Table of contents (15 chapters)

  1. Measuring Stars

  2. Equations and Processes

  3. Stellar Models

  4. Dynamical Systems

Keywords

About this book

An Introduction to the Evolution of Single and Binary Stars provides physicists with an understanding of binary and single star evolution, beginning with a background and introduction of basic astronomical concepts. Although a general treatment of stellar structure and evolution is included, the text stresses the physical processes that lead to stellar mass compact object binaries that may be sources of observable gravitational radiation.

Basic concepts of astronomy, stellar structure and atmospheres, single star evolution, binary systems and mass transfer, compact objects, and dynamical systems are covered in the text. Readers will understand the astrophysics behind the populations of compact object binary systems and have sufficient background to delve deeper into specific areas of interest. In addition, derivations of important concepts and worked examples are included. No previous knowledge of astronomy is assumed, although a familiarity with undergraduate quantum mechanics, classical mechanics, and thermodynamics is beneficial.

Authors and Affiliations

  • Texas, Department of Physics and Astronomy, University of Texas at Brownsville, Brownsville, USA

    Matthew Benacquista

About the author

Matthew Benacquista, University of Texas at Brownsville, Brownsville, USA, benacquista@phys.utb.edu

Bibliographic Information

Publish with us