The expansion of H II regions.
H II regions expansion around O, B and A stars due to interstellar hydrogen ionization by stellar radiation absorption
Axford, W. I.↗
Engineering topics
Publications and source records attributed to Newman, R. C..
H II regions expansion around O, B and A stars due to interstellar hydrogen ionization by stellar radiation absorption
Stellar wind model taking into account recombination of ionized hydrogen, noting applications to nonexpanding planetary nebulas
Ionization fronts stability, finding no instabilities for strong D type fronts
Closed form solution expressing transonic flow in idealized stellar wind and spherical accretion problems including viscosity and thermoconductivity effects