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The Brightest Binaries (Paperback, Softcover reprint of the original 1st ed. 1998)
Loot Price: R1,576
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The Brightest Binaries (Paperback, Softcover reprint of the original 1st ed. 1998)
Series: Astrophysics and Space Science Library, 232
Expected to ship within 10 - 15 working days
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Massive stars are distributed all over the upper part of the
Hertzsprung-Russell diagram according to their subsequent phases of
stellar evolution from main sequence to supernova. Massive stars
may either be single or they may be a component of a close binary.
The observed single star/binary frequency is known only in a small
part of the Galaxy. Whether this holds for the whole galaxy or for
the whole cosmos is questionable and needs many more high quality
observations.Massive star evolution depends critically on mass loss
by stellar wind and this stellar wind mass loss may change
dramatically when stars evolve from one phase to another. We start
the book with a critical discussion of observations of the
different types of massive stars, observations that are of
fundamental importance in relation to stellar evolution, with
special emphasis on mass loss by stellar wind. We update our
knowledge of the physics that models the structure and evolution of
massive single stars and we present new calculations. The
conclusions resulting from a comparison between these calculations
and observations are then used to study the evolution of massive
binaries. This book provides our current knowledge of a great
variety of massive binaries, and hence of a great variety of
evolutionary phases. A large number of case studies illustrates the
existence of these phases. Finally, we present the results of
massive star population number synthesis, including the effect of
binaries. The results indicate that neglecting them leads to a
conclusion which may be far from reality. This book is written for
researchers in massive star evolution. We hope that, after reading
this book, university-level astrophysicsstudents will become
fascinated by the exciting world of the Brightest Binaries'.
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