Subrahmanyan Chandrasekhar FRS (/ˌtʃændrəˈʃeɪkər/;[3] 19 October 1910 – 21 August 1995)[4] was an Indian-American theoretical physicist who spent his professional life in the United States. He shared the 1983 Nobel Prize for Physics with William A. Fowler for "...theoretical studies of the physical processes of importance to the structure and evolution of the stars". His mathematical treatment of stellar evolution yielded many of the current theoretical models of the later evolutionary stages of massive stars and black holes.[5][6] Many concepts, institutions, and inventions, including the Chandrasekhar limit and the Chandra X-Ray Observatory, are named after him.
<p><span style="color: rgb(33, 37, 41); font-family: system-ui, -apple-system, "Segoe UI", Roboto, "Helvetica Neue", Arial, "Noto Sans", "Liberation Sans", sans-serif, "Apple Color Emoji", "Segoe UI Emoji", "Segoe UI Symbol", "Noto Color Emoji"; letter-spacing: 0.7px;">This handy book attempts to provide most important information in clear, short and capsular form so that the student can review the subject thoroughly and prepare confidently to face the examinations. This book, first of its kind in physiology, aims to be immensely helpful to the undergraduate students as a complete guide in bulking a broad base and preparing strongly for the professional examination. The second edition has been fully revised, updated and enlarged to fulfill the current requirements of the students.</span><br></p>
