Salaris, Maurizio / Cassisi, Santi Evolution of Stars and Stellar Populations
1. Edition - October 2005 51.90 Euro 2005. 386 Pages, Softcover - Practical Approach Book - ISBN-10: 0-470-09220-3 ISBN-13: 978-0-470-09220-0 - John Wiley & Sons
Short description Evolution of Stars and Stellar Populations offers a comprehensive coverage of the links between the theory of stellar evolution and its applications to the study of stellar populations in galaxies. The book is unique in its approach as there are few if any other texts currently on the market that offer a self-contained text introducing the theory of stellar evolution first, followed by the related techniques that are widely applied by researchers in order to study stellar populations in galaxies. The presentation of stellar evolution theory is clearly presented with particular emphasis placed on the explanations of the photometric and chemical properties of stars along their evolution as a function of their initial mass and chemical composition.
From the contents Preface.
1 Stars and the Universe.
1.1Setting the stage.
1.2 Cosmic Kinematics.
1.3 Cosmic Dynamics.
1.4 Particles - and nucleosynthesis.
1.5 CMB fluctuations and structure formation.
1.6 Cosmological Parameters.
1.7 The inflationary Paradigm.
1.8 The role of Stellar Evolution.
2 Equation of state of the Stellar matter.
2.1 Physical conditions of the stellar matter.
3 Equations of stellar structure.
3.1 Basic assumptions[.
3.2 Method of solution of the stellar structure equations.
3.3 Non-standard physical process.
4 Star formation and evolution.
4.1 Overall picture of stellar evolution.
4.2 Star formation.
4.3 Evolution along the Hayashi track.
5 The hydrogen burning phase.
5.1 Overview.
5.2 The nuclear reactions.
5.3 The central H-burning phase in low main sequence stars.
5.4 The central H-burning phase in upper main sequence stars.
5.5 The dependence of MS tracks on chemical composition and convection efficiency.
5.6 Very low-mass stars.
5.7 The mass - Luminosity relations.
5.8 The Schonberg-Chandrasekhar limit.
5.9 Post-main sequence evolution.
5.10 Dependence of the main RGB features of physical and chemical parameters.
5.11 Evolutionary properties of very metal-poor stars.
6 The helium burning phase.
6.1 Introduction.
6.2 The nuclear reactions.
6.3 The zero age horizontal branch.
6.4 The core He-burning phase in low mass stars.
6.5 The central He-burning phase in more massive stars.
6.6 Pulsational properties of core He-burning stars.
7 The advanced evolutionary phase.
7.1 Introduction.
7.2 The asymptotic giant branch.
7.3 The Chandrasekhar limit and the evolution of stars with large CO cores.
7.4 carbon-oxygen white dwarfs.
7.5 The advanced evolutionary stages of massive stars.
7.6 Type la supernovae.
7.7 Neutron stars.
7.8 Black holes.
8 From theory to observations.
8.1 Spectroscopic notation of the stellar chemical composition.
8.2 From stellar models to observed spectra and magnitudes.
8.3 The effect of interstellar extinction.
8.4 K-correction for high red-shift objects.
8.5 Some general comments about colour-magnitude-diagrams.
