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Characterizing the luminosity components of luminous infrared galaxies in multi-wavelength from the X-ray to the far-infrared. [PDF]
Sci RepAli AAM +3 more
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Terrestrial atmospheric ion implantation occurred in the nearside lunar regolith during the history of Earth's dynamo. [PDF]
Commun Earth EnvironParamanick S +3 more
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Precipitation induced by explosive volcanism on Mars and its implications for unexpected equatorial ice. [PDF]
Nat CommunHamid SS, Kerber L, Clarke AB.
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Coronal dimmings and what they tell us about solar and stellar coronal mass ejections. [PDF]
Living Rev Sol PhysVeronig AM +12 more
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The dramatic transition of the extreme Red Supergiant WOH G64 to a Yellow Hypergiant
Munoz-Sanchez G +10 more
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Science, 1980
The hottest and most luminous stars lose a substantial fraction of their mass in strong stellar winds. These winds not only affect the evolution of the star, they also carve huge expanding cavities in the surrounding interstellar medium, possibly affecting star formation. The winds are probably driven by radiation pressure, but uncertainties persist in
P S Conti, R Mccray
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The hottest and most luminous stars lose a substantial fraction of their mass in strong stellar winds. These winds not only affect the evolution of the star, they also carve huge expanding cavities in the surrounding interstellar medium, possibly affecting star formation. The winds are probably driven by radiation pressure, but uncertainties persist in
P S Conti, R Mccray
exaly +3 more sources
Publications of the Astronomical Society of the Pacific, 1980
The effect of the radiative cooling on the steady-state transonic wind model is calculated. It happens that there exists a maximum limit to the mass-loss rate such that if the limit is exceeded, the wind will no longer be in the steady state and turbulence may occur, giving rise to a possible source of X rays in T Tauri objects.
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The effect of the radiative cooling on the steady-state transonic wind model is calculated. It happens that there exists a maximum limit to the mass-loss rate such that if the limit is exceeded, the wind will no longer be in the steady state and turbulence may occur, giving rise to a possible source of X rays in T Tauri objects.
openaire +1 more source