Mass loss by hot stars
Luminous hot stars mass loss attributed to negative effective gravities in outer parts of reversing layers from ionic UV resonance lines
Lucy, L. B.↗
Engineering topics
Solomon, P. M.
Publications and source records attributed to Solomon, P. M..
Molecular and solid hydrogen in dense interstellar clouds
Molecular and solid hydrogen in dense interstellar clouds suggested from underabundance of neutral atomic hydrogen, discussing grain temperature
Solomon, P. M.↗
Production of OH molecules in interstellar shock waves.
OH molecule production in interstellar shock waves, discussing rapid hydrogen production on grains
Aannestad, P. A.↗
Formation and chemical pumping of OH molecules.
Maser amplification as intense OH lines cause in small radiation sources, discussing OH molecules formation and chemical pumping
Solomon, P. M.↗
Opacity of the Venus atmosphere.
Contribution of collision induced Fermi resonance band of carbon dioxide to Venus atmosphere opacity
Solomon, P. M.↗
Mass Loss by Hot Stars
Mechanism explaining mass loss for luminous hot stars using ultraviolet line spectra of some ions
Lucy, L. B.↗
The absorption coefficient of quasi-molecular hydrogen.
Absorption coefficient of quasi-molecular hydrogen under thermodynamic equilibrium conditions
Solomon, P. M.↗