In recent years, significant advances have been made in the numerical simulation of mass-transfer processes of binary stars. These are dealt with concisely in Mass Transfer in Close Binary Stars: Gas Dynamical Treatment. Intended for specialists and postgraduates in the fields of astrophysics, observational astronomy and stellar evolution, the book covers background theory and sets out basic principles, giving many practical examples. It then offers a brief review of the available observational evidence of mass transfer in binaries. It will be useful for graduate and postgraduate students training in astrophysics as well as qualified teachers, curious to know more about the processes occurring in binary stars.
Sprache
Verlagsort
Zielgruppe
Für höhere Schule und Studium
Für Beruf und Forschung
Maße
Höhe: 254 mm
Breite: 178 mm
Gewicht
ISBN-13
978-0-415-27353-4 (9780415273534)
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Schweitzer Klassifikation
Autor*in
Russian Academy of Sciences, Moscow
Russian Academy of Sciences, Moscow
Keldysh Institute of Applied Mathematics, Moscow, Russia
Keldysh Institute of Applied Mathematics, Moscow, Russia
1. Introduction. Model of Mass Transfer in Binaries. Numerical Methods for Astrophysical Gas Flows. Mass Transfer Driven by Roche lobe Overflow. Appendix A. The Impact of Tidal Distortion of the Components' Form upon the Orbital Evolution of Binary Neutron Stars. Calculations of the Gravitational Signal. Appendix B. Equilibrium Gaseous Configurations in the Vicinity of the Gravity Centre. Appendix C. The Notation for Euler Equations in Various Coordinate Systems. Appendix D. Isothermal Gas Dynamics References. Index.