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Click the serial number on the left to view the details of the item. |
| # |
Author | Title | Accn# | Year | Item Type | Claims |
| 1 |
James Lequeux |
Birth, evolution and death of stars: An Introduction to.. |
025257 |
2013 |
Book |
|
| 2 |
Icko Iben |
Stellar evolution physics Vol. 1: Physical Processes in Stelar Interiors |
024693 |
2013 |
Book |
|
| 3 |
Icko Iben |
Stellar evolution physics Vol. 2: Advanced Evolution of Single Stars |
024694 |
2013 |
Book |
|
| 4 |
Michael Inglis |
Observer's guide to stellar evolution: The Birth, Life and Death of Stars |
024682 |
2003 |
Book |
|
| 5 |
Giora Shaviv |
Life of stars: Controversial inception and emergence of the theory of stellar structure |
023583 |
2009 |
Book |
|
| 6 |
Roger J. Tayler |
Stars: Their structure and evolution |
008565 |
1970 |
Book |
|
| 7 |
Iosif S. Shklovskii |
Stars: Their birth, life, and death |
008543 |
1978 |
Book |
|
| 8 |
Hubert Reeves |
Stellar evolution and nucleosynthesis |
003805 |
1968 |
Book |
|
| 9 |
Donald D. Clayton |
Principles of stellar evolution and nucleosynthesis |
017400 |
1983 |
Book |
|
| 10 |
Dina Prialnik |
Introduction to the theory of stellar structure and evolution |
016734 |
2000 |
Book |
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1.
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| Title | Birth, evolution and death of stars: An Introduction to.. |
| Author(s) | James Lequeux |
| Publication | Singapore, World Scientific Publishing Co. Pvt. Ltd., 2013. |
| Description | 164p. |
| Abstract Note | It has been known for a long time that stars are similar to our Sun. But it was only in 1810 that they were shown to be made of an incandescent gas. The chemical composition of this gas began to be determined in 1860. In 1940, it was demonstrated that the energy radiated by the stars is of thermonuclear origin. How stars form from interstellar matter and how they evolve and die was understood only recently, with our knowledge still incomplete. It was also realized recently that close double stars present a wide variety of extraordinary phenomena, which are far from being completely explored.
This book explains all these aspects, and also discusses how the evolution of stars determine that of galaxies. The most interesting observations are illustrated by spectacular images, while the theory is explained as simply as possible, without however avoiding some mathematical or physical developments when they are necessary for a good understanding of what happens in stars. Without being a textbook for specialists, this book can be profitably read by students or amateurs possessing some basic scientific knowledge, who would like to be initiated in-depth to the fascinating world of stars.
The author, an emeritus astronomer of the Paris Observatory, worked in various domains of astronomy connected with the subject of this book: interstellar matter and evolution of stars and galaxies. He directed the Marseilles observatory from 1983 to 1988 and served for fifteen years as Chief Editor of the professional European journal Astronomy & Astrophysics. He has written many articles and books about physics and astronomy at different levels. |
| ISBN,Price | 9789814508773 : US $26.00(PB) |
| Classification | 524.3-54
|
| Keyword(s) | 1. DOUBLE STARS
2. STAR BIRTH
3. STAR DEATH
4. STAR FORMATION
5. STARS
6. STARS - EVOLUTION
|
| Item Type | Book |
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 025257 |
|
524.3-54/LEQ/025257 |
Issued |
GP03: Piyali Ganguly |
08/May/2023 |
|
+Copy Specific Information |
2.
 |
|
| Title | Stellar evolution physics Vol. 1: Physical Processes in Stelar Interiors |
| Author(s) | Icko Iben |
| Publication | Cambridge, Cambridge University Press, 2013. |
| Description | xvi, 889 |
| Abstract Note | This text describes the microscopic physics operating in stars and demonstrates how stars respond from formation, through hydrogen-burning phases, up to the onset of helium burning. Intended for beginning graduate students and senior undergraduates with a solid background in physics, it illustrates the intricate interplay between the microscopic physical processes and the stars' macroscopic responses. The volume starts with the gravitationally contracting phase which carries the star from formation to the core hydrogen-burning main sequence, through the main sequence phase, through shell hydrogen-burning phases as a red giant, up to the onset of core helium burning. Particular emphasis is placed on describing the gravothermal responses of stars to nuclear transformations in the interior and energy loss from the surface, responses which express the very essence of stellar evolution. The volume is replete with many illustrations and detailed numerical solutions to prepare the reader to program and calculate evolutionary models. |
| ISBN,Price | 9781107016569 : UKP 95.00[Set](HB) |
| Classification | 524.3-54
|
| Keyword(s) | 1. EBOOK
2. EBOOK - CAMBRIDGE UNIVERSITY PRESS
3. EVOLUTION OF STARS
4. NEUTRINO PHYSICS
5. STELLAR DYNAMICS
6. STELLAR EVOLUTION
7. STELLAR INTERIORS
|
| Item Type | Book |
Multi-Media Links
Click Here for Online Book
Circulation Data
| Accession# | |
Call# | Status | Issued To | Return Due On | Physical Location |
| 024693 |
|
524.3-54/IBE/024693 |
On Shelf |
|
|
|
| OB0505 |
|
524.3-54/IBE/ |
On Shelf |
|
|
|
+Copy Specific Information | |