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Nucleosynthesis and chemical evolution of galaxies /

Pagel introduces a broad spectrum of astrophysics topics, from thermonuclear reactions and cosmological element production to abundance measurements in astronomical sources, nucleosynthesis, light element production by cosmic rays and stellar evolution.

Detalles Bibliográficos
Clasificación:Libro Electrónico
Autor principal: Pagel, B. E. J. (Bernard Ephraim Julius)
Formato: Electrónico eBook
Idioma:Inglés
Publicado: Cambridge : Cambridge University Press, Ã2009.
Edición:2nd ed.
Temas:
Acceso en línea:Texto completo

MARC

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100 1 |a Pagel, B. E. J.  |q (Bernard Ephraim Julius) 
245 1 0 |a Nucleosynthesis and chemical evolution of galaxies /  |c Bernard Pagel. 
250 |a 2nd ed. 
260 |a Cambridge :  |b Cambridge University Press,  |c Ã2009. 
300 |a 1 online resource (xvii, 466 pages) :  |b illustrations 
336 |a text  |b txt  |2 rdacontent 
337 |a computer  |b c  |2 rdamedia 
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500 |a Previous edition: 1997. 
504 |a Includes bibliographical references (pages 431-452) and index. 
505 0 |a Introduction and overview -- Thermonuclear reactions -- Cosmic abundances of elements and isotopes -- Cosmological nucleosynthesis and abundances of light elements -- Outline of stellar structure and evolution -- Neutron capture processes -- Galactic chemical evolution : basic concepts and issues -- Some specific GCE models and related observational data -- Origin and evolution of light elements -- Radioactive cosmochronology -- Chemical evolution in other sorts of galaxies -- Cosmic chemical evolution and diffuse background radiation -- Appendix 1: Some historical landmarks -- Appendix 2: Some physical and astronomical constants -- Appendix 3: Time-dependent perturbation theory and transition probabilities -- Appendix 4: Polytropic stellar models -- Appendix 5: Dissipation and abundance gradients -- Appendix 6: Hints for problems. 
520 |a Pagel introduces a broad spectrum of astrophysics topics, from thermonuclear reactions and cosmological element production to abundance measurements in astronomical sources, nucleosynthesis, light element production by cosmic rays and stellar evolution. 
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