Red supergiants and neutrino emission.
Red supergiants as old derivatives of main sequence O and B stars, discussing neutrino emissions and carbon core contraction
Stothers, R.↗
Engineering topics
Stothers, R.
Publications and source records attributed to Stothers, R..
Pulsational instabilities in hydrogen-poor massive blue stars. I.
Structure and pulsational properties of massive stars with helium cores and thin hydrogen poor envelopes
Simon, N. R.↗
Massive stars
Normal O, blue supergiants and brightest yellow and red supergiant massive stars, considering evolution, luminosity, lifetime mass loss, pulsational instability and supernovae
Stothers, R.↗
Ultraviolet dwarfs and planetary nebulae
UV dwarfs observational lifetime, considering progenitor main sequence, red giants and planetary nebulae central stars evolutionary sequence
Stothers, R.↗
An interpretation of the peculiar helium star HZ 29.
Variable He star HZ29, noting unusually wide and shallow He I lines and possible mass and composition
Stothers, R.↗
Evolution of massive helium-burning supergiants.
Massive supergiant star models construction for core He plasma burning evolution phase, discussing luminosity and temperature sensitivity to internal instability
Chin, C.-W.↗
On the pulsational stability of blue supergiants.
Blue supergiant stars pulsational stability and brightness constancy using model interiors, considering surface shell energy source and stellar evolution implications
Simon, N. R.↗
On the pulsation hypothesis for massive red supergiants
Red supergiant pulsar hypothesis using Q values derived from stellar luminosity, period, and spectrum
Stothers, R.↗
An interpretation of the peculiar helium star HZ 29
Radial pulsation model for helium-burning main sequence star
Stothers, R.↗
Pulsational Instabilities in Hydrogen-poor Massive Blue Stars. 1
Structure and pulsational properties of hydrogen poor massive blue stars with helium cores
Simon, N. R.↗
Evolution of a star of 30 solar masses.
Evolution sequence of 30 solar mass stellar models, discussing structural and nuclear evolution
Stothers, R.↗
A criterion for nuclear-energized pulsational instability
Explore the source record for details and available documents.
Simon, N. R.↗
The linear star model and dynamical instability.
Pulsation properties of star models with linear density distribution, considering radial, adiabatic contraction and dynamical stability
DENSITY DISTRIBUTION↗
Astrophysical evidence for the direct electron- neutrino weak interaction.
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
Chin, C.-W.↗
The ultraviolet dwarfs - A new class of degenerate stars.
Plasma neutrino process as accelerating mechanism for evolution in UV dwarfs
ULTRAVIOLET PHOTOMETRY↗
Astrophysical evidence for the direct electron-neutrino weak interaction.
Plasma neutrino process of Adams, Ruderman and Woo dependent on direct electron-neutrino interaction and connected with stellar evolution
NEUTRINO↗
The semiconvective zone in very massive stars.
Semiconvective zone in very massive stars during hydrogen burning, noting factors leading to instability
STELLAR STRUCTURE↗