Lecture Notes on Stellar Structure and Evolution Jørgen Christensen-Dalsgaard Institut for Fysik og Astronomi, Aarhus Universitet Sixth Edition Fourth Printing March 2008 ii Preface The present notes grew out of an introductory course in stellar evolution which I have given for several years to third-year undergraduate students in physics at the University of Aarhus. The goal of the course and the notes is to show how many aspects of stellar evolution can be understood relatively simply in terms of basic physics. Apart from the intrinsic interest of the topic, the value of such a course is that it provides an illustration (within the syllabus in Aarhus, almost the first illustration) of the application of physics to “the real world” outside the laboratory. I am grateful to the students who have followed the course over the years, and to my colleague J. Madsen who has taken part in giving it, for ments and advice; indeed, their insistent urging that I replace by a more coherent set of notes the textbook, supplemented by mentary and additional notes, which was originally used in the course, is directly responsible for the existence of these notes. Additional input was provided by the students who suffered through the first edition of the notes in the Autumn of 1990. I hope that this will be a continuing process; ments, corrections and suggestions for improvements are most e. I thank N. Grevesse for providing the data in Figure , and P. E. Nissen for helpful suggestions for other figures, as well as for reading menting on an early version of the manuscript. I also thank Bent Christensen-Dalsgaard and T. M. Brown for their assistance in locating the Bradbury reference in Chapter 2. The High Altitude Observatory, Boulder, Colorado is thanked for hospitality during the Summer of 1990, where a substantial part of the notes were written. Aarhus, August 1991 Jørgen Christensen-Dalsgaard Preface to 4th edition Relative to earlier edi
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