The structure and evolution of stars (Record no. 72850)
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000 -LEADER | |
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fixed length control field | 02721nmm a2200373 a 4500 |
001 - CONTROL NUMBER | |
control field | 0000p974 |
005 - DATE AND TIME OF LATEST TRANSACTION | |
control field | 20220711214231.0 |
008 - FIXED-LENGTH DATA ELEMENTS--GENERAL INFORMATION | |
fixed length control field | 190115s2019 si a ob 001 0 eng |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
ISBN | 9781783265817 |
-- | (ebook) |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
-- | (hbk.) |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
-- | (hbk.) |
020 ## - INTERNATIONAL STANDARD BOOK NUMBER | |
-- | (pbk.) |
082 04 - CLASSIFICATION NUMBER | |
Call Number | 523.8/8 |
100 1# - AUTHOR NAME | |
Author | Eldridge, J. J. |
245 14 - TITLE STATEMENT | |
Title | The structure and evolution of stars |
260 ## - PUBLICATION, DISTRIBUTION, ETC. (IMPRINT) | |
Place of publication | Singapore : |
Publisher | World Scientific Publishing Co. Pte Ltd., |
Year of publication | ©2019. |
300 ## - PHYSICAL DESCRIPTION | |
Number of Pages | 1 online resource (360 p.) : |
520 ## - SUMMARY, ETC. | |
Summary, etc | "Stars are the fundamental observable constituents of the Universe. They are the first objects we see in the night sky, they dominate the light produced in our own and other galaxies, and nucleosynthesis in stars produces all the elements heavier than helium. A knowledge of stars and their evolution is vital to understand other astrophysical objects from accreting black holes and galaxies to the Universe itself. The structure of a star can be described mathematically by differential equations derived from the principles of hydrodynamics, electromagnetic theory, thermodynamics, quantum mechanics, atomic and nuclear physics. The basic equations of a spherical star are derived in detail at an accessible level. The topics discussed include modes of energy transport, the equation of state, the physics of the opacity sources and the nuclear reactions. Attention is also given to the virial theorem, polytropic gas spheres and homology principles and the procedure for numerical solution of the equations is outlined. This book tracks the evolution of stars from their main-sequence evolution through the exhaustion of various nuclear fuels to the end points of evolution and also introduces the topic of interacting binary stars. The aim is to take the reader from the essential underlying physical principles to the doors to current research on stellar interiors."-- |
650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
General subdivision | Formation. |
650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
General subdivision | Evolution. |
700 1# - AUTHOR 2 | |
Author 2 | Tout, Christopher A. |
856 40 - ELECTRONIC LOCATION AND ACCESS | |
Uniform Resource Identifier | https://www.worldscientific.com/worldscibooks/10.1142/p974#t=toc |
942 ## - ADDED ENTRY ELEMENTS (KOHA) | |
Koha item type | eBooks |
588 ## - | |
-- | Title from web page (viewed January 15, 2019). |
520 ## - SUMMARY, ETC. | |
-- | Publisher's website. |
650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
-- | Stars |
650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
-- | Stars |
650 #0 - SUBJECT ADDED ENTRY--SUBJECT 1 | |
-- | Electronic books. |
No items available.