Evolution of O stars. III - Helium burning.
Stellar evolution for star of 30 solar masses during helium ignition, depletion and exhaustion
Engineering topics
Publications and source records attributed to Stothers, R..
Stellar evolution for star of 30 solar masses during helium ignition, depletion and exhaustion
Mixed star evolution, mass loss and mass- luminosity-mean molecular weight relation
Quasars creation of matter in steady state expanding universe
Three postulates relating radio star galaxies, quasars and spontaneous creation of energy mass
Low rotational velocities and period analyses of Beta Cephei variables lead to hypothesis that they are nonrotating stars undergoing radial oscillations
Evolution of giant star from helium ignition through helium exhaustion - astrophysics
Theory of evolution of completely mixed stars with mass loss - prediction of luminosity function
Semiconvective zone and convective core as function of stellar mass and evolution during hydrogen burning
Astrophysical evidence for direct electron- neutrino weak interaction - theoretical models of superluminous white dwarfs with and without neutrino emission process
O stars from early phase of hydrogen burning to hydrogen exhaustion and gravitational attraction preceding helium burning
Evolution of o stars - hydrogen exhaustion and gravitational contraction
Analysis of spatial distribution of rv tauri stars in field and comparison with similar stars found in globular clusters
Evolutionary state of beta Cephei variable stars
Correlation of frequency of occurence of super- novae with theories of mass loss and neutrino emission from red giants
O-star evolution from initial main sequence state to point of decreased hydrogen core content
Neutrino emission on element abundances in stars