Volume 2 contains the basic physical ideas and laws used in the study of the outer layers of a star including stellar magnitudes, spectra and temperatures, radiative transfer in a stellar atmosphere, line formation, the spectrum of hydrogen, spectral analysis, and available structural components.
Introduction to stellar astrophysics,
β Scribed by Boehm-Vitense E.
- Publisher
- CUP
- Year
- 1997
- Tongue
- English
- Leaves
- 303
- Edition
- 3pr
- Category
- Library
No coin nor oath required. For personal study only.
β¦ Synopsis
This book is the final one in a series of three texts which together provide a modern, complete and authoritative account of our present knowledge of the stars. It discusses the internal structure and the evolution of stars, and is completely self-contained. There is an emphasis on the basic physics governing stellar structure and the basic ideas on which our understanding of stellar structure is based. The book also provides a comprehensive discussion of stellar evolution. Careful comparison is made between theory and observation, and the author has thus provided a lucid and balanced introductory text for the student. As for volumes 1 and 2, volume 3 is self-contained and can be used as an independent textbook. The author has not only taught but has also published many original papers in this subject. Her clear and readable style should make this text a first choice for undergraduate and beginning graduate students taking courses in astronomy and particularly in stellar astrophysics.
β¦ Subjects
Π€ΠΈΠ·ΠΈΠΊΠ°;ΠΡΡΡΠΎΠ½ΠΎΠΌΠΈΡ ΠΈ Π°ΡΡΡΠΎΡΠΈΠ·ΠΈΠΊΠ°;ΠΡΡΡΠΎΡΠΈΠ·ΠΈΠΊΠ°;ΠΡΡΡΠΎΡΠΈΠ·ΠΈΠΊΠ° Π·Π²Π΅Π·Π΄;
π SIMILAR VOLUMES
This textbook introduction to the basic elements of fundamental astronomy and astrophysics serves as a foundation for understanding the structure, evolution, and observed properties of stars. The first half of the book explains how stellar motions, distances, luminosities, colors, radii, masses and
Volume 2 contains the basic physical ideas and laws used in the study of the outer layers of a star including stellar magnitudes, spectra and temperatures, radiative transfer in a stellar atmosphere, line formation, the spectrum of hydrogen, spectral analysis, and available structural components.
An 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
An 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
<b><i>An Introduction to Stellar Astrophysics</i></b> 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.<p>The book is divided into seven chapters, fea