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Woosley, Stanford E.

Overview
Works: 25 works in 80 publications in 4 languages and 969 library holdings
Genres: Conference papers and proceedings 
Roles: Author, Editor, Other
Classifications: QB471.7.B85, 522.6862
Publication Timeline
Key
Publications about Stanford E Woosley
Publications by Stanford E Woosley
Most widely held works about Stanford E Woosley
 
Most widely held works by Stanford E Woosley
High energy transients in astrophysics (Santa Cruz, CA, 1983) ( Book )
11 editions published in 1984 in English and Undetermined and held by 273 libraries worldwide
Supernovae : the Tenth Santa Cruz Workshop in Astronomy and Astrophysics, July 9 to 21, 1989, Lick Observatory by Stanford E Woosley( Book )
15 editions published in 1991 in English and held by 220 libraries worldwide
Supernova explosions are not only important to the ecology of the universe, seeding it, among other things, with the heavy elements necessary for the existence of life, but they are also a natural laboratory in which a host of unique physical phenomena occur. While still far from a complete understanding, scientists have made great advances during the last twenty-five years in understanding the nature and conse- quences of supernovae. This book presents the state of supernova studies at the beginning of the 1990's, as reported at a two-week meeting on the Santa Cruz campus of the University of California in July 1989 in- volving 177 astronomers and astrophysicists from 17 nations. The 110 papers contained in this volume report all aspects of the field - observations at all wavelengths from radio through gamma-rays, bolometric light curves and spectra, neutrino observations, the theory of stellar explosions, multidimensional models for mixing, nucleosynthesis calculations, synthetic spectral modeling, presupernova evolution, supernova remnants, supernova rates, supernovae as standard candles, the interaction of supernovae with their surroundings - and constitute the most comprehensive and up-to-date treatment of SN 1987A currently available. Astronomers and astronomy graduate students will find this an in valuable summary of the current state of supernova research. The informed layperson or undergraduate astronomy student will also find it a useful introduction and guide to the literature in the subject
Gamma-ray bursts : Huntsville, Al., 1991 by William Simon Paciesas( Book )
8 editions published in 2012 in English and held by 107 libraries worldwide
La 4e de couv. indique : "Cosmic gamma ray bursts (GRBs) have fascinated scientists and the public alike since their discovery in the late 1960s. Their story is told here by some of the scientists who participated in their discovery and, after many decades of false starts, solved the problem of their origin. Fifteen chapters by active researchers in the field present a detailed history of the discovery of GRBs, a comprehensive theoretical description of GRB central-engine and emission models, a discussion of GRB host galaxies, a guide to how GRBs can be used as cosmological tools, and critical thougts on the future of the field. Observations are grouped into three sets from the satellites CGRO, BeppoSAX and Swift, and are followed by a discussion of multiwavelength observations ; the first results of Fermi on GRBs are described in various chapters. This is the first edited volume on GRB astrophysics that presents a fully comprehensive review of the subject. Utilizing the latest research, Gamma-ray Bursts is an essential desktop companion for graduate students and researchers in astrophysics"
High energy transients : final technical report to the National Aeronautics and Space Administration by Summer Workshop in Astronomy & Astrophysics( Book )
1 edition published in 1984 in English and held by 54 libraries worldwide
The explosive burning of oxygen and silicon by Stanford E Woosley( Book )
2 editions published in 1973 in English and held by 23 libraries worldwide
Nuclear astrophysics : proceedings of the Caltech Centennial Year Nuclear Astrophysics Symposium in honor of William A. Fowler's 80th birthday by Nuclear Astrophysics Symposium( Book )
6 editions published in 1993 in English and held by 22 libraries worldwide
Neutron-rich nucleosynthesis in carbon deflagration supernovae by Stanford E Woosley( file )
1 edition published in 1999 in English and held by 6 libraries worldwide
Nucleosynthesis during advanced burning stages of stars by Stanford E Woosley( Archival Material )
2 editions published in 1982 in English and held by 4 libraries worldwide
Semiempirical thermonuclear reaction-rate data for intermediate-mass nuclei ( Book )
1 edition published in 1978 in English and held by 3 libraries worldwide
A new twist on neutron stars by Chris Fryer( Article )
1 edition published in 2001 in English and held by 1 library worldwide
Children of the stars : how the violent death of stars creates conditions for life in the universe by Stanford E Woosley( Sound Recording )
1 edition published in 2008 in English and held by 1 library worldwide
The great supernova of 1987 by Stanford E Woosley( Article )
1 edition published in 1989 in English and held by 1 library worldwide
Gamma-ray line signals from supernovae within 100 Mpc¹ ( Book )
1 edition published in 1997 in English and held by 1 library worldwide
Tables of thermonuclear reaction rate data for intermediate mass nuclei by Stanford E Woosley( Book )
1 edition published in 1975 in English and held by 1 library worldwide
Supernovae The Tenth Santa Cruz Workshop in Astronomy and Astrophysics, July 9 to 21, 1989, Lick Observatory by Stanford E Woosley( file )
1 edition published in 1991 in English and held by 1 library worldwide
High energy transients in astrophysics: Aip conference proceedings ( Book )
1 edition published in 1984 in Italian and held by 1 library worldwide
Nuclear data needs for the study of nucleosynthesis in massive stars ( file )
1 edition published in 2003 in English and held by 1 library worldwide
The critical nuclear physics needed to calculate the evolution of and nucleosynthesis in massive stars is reviewed with emphasis on the uncertainties. Some reaction rates - the most important and uncertain still being C-12 (alpha, gamma)O-16 - are important for energy generation and stellar structure. Others, like Ne-22(alpha,n)Mg-25 and individual cross sections for neutron capture determine the overall yield and distribution of the s-process for elements lighter than A = 90. Still others affect the synthesis of individual nuclei, e.g., by the nu-process, the rp-process, and the gamma-process. Weak interaction rates are important in determining the structure of both the pre-collapse and the post-collapse supernova core. Finally, both the site for, and the nuclear physics of the r-process remains very uncertain, quite possibly because of the neglect of magnetic fields
La gran supernova de 1987 by Tom Weaver( Article )
1 edition published in 1989 in Spanish and held by 1 library worldwide
Prompt and Afterglow Emission Properties of Gamma-Ray Bursts with Spectroscopically Identified Supernovae ( file )
1 edition published in 2006 in English and held by 0 libraries worldwide
We present a detailed spectral analysis of the prompt and afterglow emission of four nearby long-soft gamma-ray bursts (GRBs 980425, 030329, 031203, and 060218) that were spectroscopically found to be associated with type Ic supernovae, and compare them to the general GRB population. For each event, we investigate the spectral and luminosity evolution, and estimate the total energy budget based upon broadband observations. The observational inventory for these events has become rich enough to allow estimates of their energy content in relativistic and sub-relativistic form. The result is a global portrait of the effects of the physical processes responsible for producing long-soft GRBs. In particular, we find that the values of the energy released in mildly relativistic outflows appears to have a significantly smaller scatter than those found in highly relativistic ejecta. This is consistent with a picture in which the energy released inside the progenitor star is roughly standard, while the fraction of that energy that ends up in highly relativistic ejecta outside the star can vary dramatically between different events
 
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Alternative Names
Stanford E. Woosley Amerikaans natuurkundige
Stanford E. Woosley amerikansk astronom och fysiker
Stanford E. Woosley amerikansk astronom og fysikar
Stanford E. Woosley amerikansk astronom og fysiker
Stanford E. Woosley US-amerikanischer Astrophysiker
Woosley, S. E.
Woosley, S. E. 1944-
Woosley, S. E. (Stanford E.)
Woosley, Stan
Woosley, Stan 1944-
Woosley, Stanford E.
Woosley, Stanford Earl 1944-
Вусли, Стэнфорд американский физик
استنفرد ای ووسلی فیزیک‌دان و ستاره‌شناس آمریکایی
Languages
English (71)
Spanish (1)
German (1)
Italian (1)
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