Results 281 to 290 of about 487,950 (322)
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Radiative opacity due to the red system of CN

Journal of Quantitative Spectroscopy and Radiative Transfer, 1972
Abstract Recent observational and theoretical work has indicated that CN may play a major role in forming the spectrum and in fixing the thermal structure in a wide variety of cool stellar atmospheres. As the first step in investigating that role, we have calculated straight mean absorption coefficients over intervals of 100 cm -1 for the red system
H. R. Johnson, I. Marenin, S. Price
semanticscholar   +2 more sources

Calculation of radiative opacity of plasma mixtures using a relativistic screened hydrogenic model

Journal of Quantitative Spectroscopy and Radiative Transfer, 2014
M. Mendoza   +7 more
semanticscholar   +3 more sources

Radiative opacity of low-Z plasma using screened hydrogenic model including l-splitting

Journal of Quantitative Spectroscopy and Radiative Transfer, 2012
M. Das, M. Srivastava, S. Menon
semanticscholar   +3 more sources

Calculation of the radiative opacity of laser-produced plasmas using a relativistic-screened hydrogenic model

Journal of Quantitative Spectroscopy and Radiative Transfer, 2004
J. G. Rubiano   +5 more
semanticscholar   +3 more sources

Radiative properties of stellar envelopes: Comparison of asteroseismic results to opacity calculations and measurements for iron and nickel

High Energy Density Physics, 2013
S. Turck-chièze   +25 more
semanticscholar   +3 more sources

Radiative opacities for stellar envelopes

Physica Scripta, 1995
Recent advances in the field of opacity calculations for stellar envelopes are summarized. The methods used and the results obtained in the last decade by two independent groups are discussed briefly. Some of the important effects of the new data on astrophysical studies are outlined.
openaire   +1 more source

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