An Introduction to Stellar AstrophysicsAn Introduction to Stellar Astrophysics aspires to provide the reader with an intermediate knowledge on stars whilst focusing mostly on the explanation of the functioning of stars by using basic physical concepts and observational results. The book is divided into seven chapters, featuring both core and optional content:
Student-friendly features include:
This book is designed to cover the most important aspects of stellar astrophysics inside a one semester (or half-year) course and as such is relevant for advanced undergraduate students following a first course on stellar astrophysics, in physics or astronomy programs. It will also serve as a basic reference for a full-year course as well as for researchers working in related fields. |
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absorbed abundance acceleration approximately assuming astronomical atmosphere atomic atomic lines average becomes calculations called caused central Chapter cloud consideration constant convective core defined density depends depth diffusion direction discussed distance effective electron elements emitted energy equal equation equilibrium evolution example exists expression field Figure flux force formed frequency function fusion galaxies given gives gravitational helium hydrogen Illustration important increases integrated inthe ionisation ions known larger layers leads luminosity magnetic magnitude main sequence mass matter mean neutrinos neutron nuclear nucleus observed obtained ofthe opacity particles period phase photons physical plasma population present pressure production pulsation quantity radiation radiative radius reaction regions relatively respect scattering seen shown shows solar specific intensity spectra spectrum stars stellar stellar atmospheres structure supernova surface temperature tothe transfer transitions transport types unit variable various white dwarfs written