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Clayton, Donald D.

Overview
Works: 28 works in 87 publications in 1 language and 3,021 library holdings
Genres: Biography  History  Maps 
Classifications: QB450, 523.02
Publication Timeline
Key
Publications about Donald D Clayton
Publications by Donald D Clayton
Most widely held works about Donald D Clayton
 
Most widely held works by Donald D Clayton
Handbook of isotopes in the cosmos hydrogen to gallium by Donald D Clayton( file )
9 editions published in 2003 in English and held by 957 libraries worldwide
An information resource about the isotopes and their place in the cosmos
Principles of stellar evolution and nucleosynthesis by Donald D Clayton( Book )
32 editions published between 1968 and 2007 in English and held by 877 libraries worldwide
The dark night sky : a personal adventure in cosmology by Donald D Clayton( Book )
4 editions published in 1975 in English and held by 623 libraries worldwide
Essays in nuclear astrophysics : presented to William A. Fowler, on the occasion of his seventieth birthday ( Book )
6 editions published between 1981 and 1982 in English and held by 292 libraries worldwide
The Joshua factor : a novel by Donald D Clayton( Book )
5 editions published between 1986 and 1988 in English and held by 172 libraries worldwide
The explosive burning of oxygen and silicon by Stanford E Woosley( Book )
2 editions published in 1973 in English and held by 24 libraries worldwide
Handbook of isotopes in the cosmos by Donald D Clayton( Book )
3 editions published in 2003 in English and held by 23 libraries worldwide
Nucleosynthesis of heavy elements by neutron capture by Philip A Seeger( Book )
3 editions published between 1964 and 1965 in English and held by 5 libraries worldwide
Nucleosynthesis of elements heavier than the iron group by neutron capture on both slow and fast time scales is evaluated. The s-process calculations of Clayton, Fowler, Hull, and Zimmerman (Ann. Phys. 12:331, 1961) were revised to include more recent experimental results on abundances and neutron capture cross-sections. The solar-system s-process abundances indicate a history of neutron exposure distributions characterized by decreasing probability of high integrated flux; an exponential exposure distribution is extracted. Estimates are made of the s-process contribution to each isotopic abundance; a table gives the amounts of elements produced by each process in the solar-system material. The r-process calculations are carried out using a semi-empirical atomic-mass law to determine neutron-binding energies and beta-decay probabilities. The solar-system r-process material has probably been synthesized in two distinct types of environments. (Author)
26Al in the interstellar medium by Donald D Clayton( Book )
2 editions published in 1987 in English and held by 5 libraries worldwide
Nuclear quasi-equilibrium during silicon burning by David Bodansky( Book )
2 editions published in 1968 in Undetermined and English and held by 4 libraries worldwide
Principles of stellar evolution and nucleosynhesis by Donald D Clayton( Book )
2 editions published between 1968 and 1983 in English and held by 3 libraries worldwide
26 Al in the interstellar medium by Donald D Clayton( Book )
1 edition published in 1987 in English and held by 3 libraries worldwide
Hydrogen to gallium by Donald D Clayton( Book )
1 edition published in 2003 in English and held by 3 libraries worldwide
Prospects for nuclear gamma-ray astronomy by Donald D Clayton( Book )
1 edition published in 1973 in English and held by 2 libraries worldwide
A walking tour of residential Seneca by Donald D Clayton( Book )
1 edition published in 2001 in English and held by 2 libraries worldwide
PRINCIPLES OF STELLAR EVOLUTION AND NUCLEOSYNTHESIS, ( Book )
1 edition published in 1969 in English and held by 1 library worldwide
The fields of stellar evolution and nucleosynthesis comprise one of the most vital and intriguing areas of modern sceintific research. The recent build-up in the space exploration program has been accompanied by a new surge of interest in the physics of natural phenomena. Since stars are the most common element in the universe, much of our knowledge is moderated by our concepts of their structure and evolution, and the synthesis of elements from which they are formed. This is the first text to present the basic physical principles of stellar evolution and nucleosynthesis. The book provides a clear statement of the ideas which dominate modern research in the hope that it will attract more students into this exciting field. By concentrating on the physical principles, the author has attempted to clarify the theoretical ideas which will prove valuable in a wide variety of future problems. (Author)
Principles of stellar evolution and nucleasynthesis by Donald D Clayton( Book )
1 edition published in 1968 in English and held by 1 library worldwide
Theoretical Nuclear Astrophysics ( Book )
1 edition published in 1970 in English and held by 1 library worldwide
The great preponderance of this research has been directed toward the many ramifications of a single problem -- to evaluate the nuclear data for and against the proposition that the chemical elements have been created by nuclear reactions in stars. Results are discussed
26Al in the interstellar region by Donald D Clayton( Article )
1 edition published in 1987 in English and held by 1 library worldwide
 
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Alternative Names
Clayton, D. D. (Donald D.)
Clayton, Donald
Klejton, D.
Klejton, D., 1935-
Languages
English (83)
Covers
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