Nucleosynthesis in Supernova Shock Waves
Thermonuclear reactions occurring in supernova shock wave propagating through stellar envelope
Engineering topics
Publications and source records attributed to Cameron, A. G. W..
Thermonuclear reactions occurring in supernova shock wave propagating through stellar envelope
Abnormal low helium abundance in atmospheres of old halo B star based on weak absorption lines in helium spectra
Astronomical observations through X-ray, ultraviolet, and radio astronomy
Rapid neutron capture in supernova explosions
Anomalous silicon abundance production in Ap stars
Neutron star vibration period and thermal, rotational, vibrational and magnetic energy storage mechanisms in supernova after envelope ejection
X-ray emission from old novae noting possibility that hot coronas may arise from vibration
Surface properties, temperature effect, cooling and detectability of neutron stars, using pure iron and pure magnesium compositions
Neutron star structure analysis using composite state equation
Neutron star rotational flattening after formation in supernova implosion
Melting of solid bodies in chondrule size, discussing accumulation mechanisms involving electrostatic acceleration and gas motions
Nuclear reaction and beta decay rates for silicon 28, considering conditions for nuclear statistical equilibrium in stars
Model sequence calculations of early solar evolution extended for case of varying-G cosmology
Earth-moon system origin assuming moon was formed from terrestrial material ejected from earth during rotational instability
Earth-moon system - NASA Goddard Institute for Space Studies, Conference, New York, January 1964
Sources of X-rays and high-energy gamma rays, including inverse Compton effect, synchrotron radiation, brehmsstrahlung from hot plasma, and decay of neutral pions
Thermonuclear reaction rates in medium and heavy nuclei determined from statistical properties